The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and rounded morphology. There is minimal discernible structure such as spiral arms or a prominent disk. The galaxy's light profile increases gradually towards the center, indicative of a centrally concentrated stellar population. The color appears to be dominated by redder wavelengths, suggesting a population of older stars and a relatively low rate of on-going star formation. Any dust content present is likely minimal, given the relatively clean color and the absence of visible dust lanes. There is no evidence of any recent merger activity or significant tidal disturbances affecting the overall structure of the galaxy.
