The galaxy presents as an elliptical structure with a relatively smooth morphology. It exhibits a concentrated central bulge that gradually diffuses outward, transitioning into a fainter halo. The color profile shows a yellowish core, suggesting a population of older stars dominating the central region. There is a slight reddening in the intermediate regions, possibly indicative of dust lanes or a mix of stellar populations. The galaxy's overall shape is elongated, deviating from a perfect sphere. There is no apparent evidence of strong spiral arms or active star-forming regions. Subtle, diffuse features might suggest minor interactions or past merger events, but no major tidal disturbances are immediately apparent.
