The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the inner region. Moving outward from the core, the color subtly shifts towards a redder tone, indicative of potentially cooler stars or increased dust extinction. There is a subtle disk-like feature, but it is not well defined, and this galaxy would largely be considered an elliptical type. There are no readily apparent spiral arms or other significant structural features such as tidal tails or signs of recent major merger events. Based on its color and smooth morphology, it is likely a relatively massive galaxy with a suppressed rate of ongoing star formation.
