The galaxy exhibits a largely smooth morphology, with a dominant spheroidal component. The light distribution appears relatively uniform and centrally concentrated, with a smooth decline in surface brightness from the core outwards. There is a slight elongation in the galaxy's shape, suggesting it is not perfectly spherical, with an intermediate elliptical appearance. Faint disturbances appear in the galaxy structure, though the image lacks the resolution to determine if this is a merger event. The galaxy's color profile indicates a redder hue, suggesting a stellar population dominated by older, evolved stars with possible dust content. The central region shows a more pronounced yellow color, possibly indicative of a dense concentration of these older stars or dust obscuration. Overall, the galaxy presents characteristics consistent with an elliptical galaxy with a high mass and low star formation rate.
