The galaxy appears to be a relatively compact object. The light is concentrated, with a brighter central region. There is evidence of a fainter, more diffuse halo surrounding this brighter core. A slight elongation is observed, indicating that the galaxy may not be perfectly spherical, perhaps slightly flattened. The color profile suggests a mix of stellar populations, the central area presenting bluer wavelengths, and some redder or yellowed light in the outer regions. This might indicate ongoing star formation closer to the core and older stellar populations further out, or a possible difference in dust content. There's an apparent disturbance or faint extension, possibly suggestive of a minor tidal interaction, although it could also be an artifact or background object partially overlapping. The overall structure lacks defined spiral arms or a prominent disk-like structure.
