The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. It exhibits a mild elongation, appearing somewhat oblate rather than perfectly spherical. The central region is the brightest, displaying a reddish hue, which may indicate a population of older stars, significant dust obscuration, or a combination of both. The outer regions show a bluer tint, suggesting the presence of a younger stellar population, although the color contrast is subtle. No prominent spiral arms or distinct features are visible. There is a possible minor disturbance in the morphology, with a slight asymmetry or irregularity on one side, however this is difficult to verify at this resolution. Overall, it looks like a fairly massive system, but it doesn't show evidence of significant ongoing star formation.
