The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular type. Its overall shape appears moderately round, with a slight deviation towards an elongated form. The central region exhibits a high concentration of light, indicative of a significant bulge component.

The galaxy's color profile shows a dominance of redder hues, particularly within the core, potentially arising from an older stellar population and lower levels of ongoing star formation. Fainter, bluer light is subtly present in the outer regions, implying the existence of younger stars though these are not dominant. No obvious spiral arms or significant dust lanes are discernible within the image. There are no obvious signs of any ongoing major merger events, although there may be some minor disturbance or interaction with the galaxy.
