The galaxy presents as a centrally concentrated, smooth object, with a primarily elliptical morphology. There is little evidence of distinct spiral arm structure or significant dust lanes. The light profile appears to gradually decrease in intensity from the core outwards, with a moderate radial color gradient. The central region exhibits a yellowish-white hue, suggestive of an older stellar population. The outer regions appear slightly redder, likely indicating a continuation of the aging stellar population. The galaxy's overall form is well-defined and shows no indications of tidal disturbances or ongoing major mergers. There are no apparent nearby companions or significant distortions in its shape that might suggest recent interactions. Overall, the galaxy is most likely an early-type galaxy, perhaps an elliptical, exhibiting a smooth and featureless appearance.
