This galaxy appears to be an interacting system, or possibly a galaxy with significant tidal features. The primary body of the galaxy exhibits an elongated morphology, suggestive of a disk viewed at a high inclination or a spheroid. A distinct redder, more compact region is observed on one side of the main body. This could be a bulge component with an older stellar population, or a separate object that is gravitationally interacting with the main galaxy. A faint extension or arc of light is also observed, potentially indicative of tidal stripping or disturbance from the interaction. The overall color profile suggests a mix of stellar populations, with the bluer hues potentially indicating ongoing star formation, and redder areas showing the presence of older stars. Dust may also play a role in reddening the light observed from the galaxy. The galaxy doesn't appear to exhibit a strong spiral structure, but could potentially have a warped or irregular disk. Further analysis of the spectral properties would be beneficial to confirm star formation rates and stellar population ages.
