The galaxy presents a somewhat diffuse morphology. It exhibits a redder hue, indicative of older stellar populations or significant dust obscuration. The overall structure suggests a non-smooth form, with potential features hinting at minor disturbances or interactions. There appears to be a slight asymmetry in its outer regions, suggesting a possible tidal interaction or recent accretion event. While a central bulge is not clearly defined, a slight concentration of luminosity may be present towards the galaxy's core. Detailed analysis and additional observations are necessary to fully characterize its structure, star formation history, and dynamical state.
