The galaxy presents as an elliptical morphology, appearing largely spheroidal with a smooth, diffuse structure. The central region exhibits a higher concentration of light, indicative of a prominent galactic nucleus. The color profile suggests a relatively older stellar population, with a yellow-orange hue dominating the core and inner regions. The outer edges show subtle bluish tints, implying the presence of younger, hotter stars, albeit in a lesser proportion compared to the core. There appears to be little or no distinct spiral arm structure or prominent dust lanes. There is no obvious indication of major mergers or significant tidal disturbances. The galaxy seems to be relatively isolated and undisturbed.
