The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a subtle yellowish hue, indicative of a dominant older stellar population and relatively low ongoing star formation. It shows an elliptical morphology, appearing somewhat rounded in shape, with only minor deviations from perfect circularity. There is no discernible spiral arm structure or prominent dust lanes visible in this image. The galaxy displays evidence of a potential minor interaction or disturbance, possibly a faint tidal feature or slight asymmetry in the outer regions of the halo. A notable fraction of light seems centrally condensed. No significant central bulge or bright nucleus is immediately apparent in the observation, though higher resolution data would be required for confirmation.
