The galaxy presents as a singular, spatially resolved object with an elliptical morphology. A dominant central bulge region is apparent, exhibiting a concentration of light that suggests a high stellar density. The galaxy displays a generally smooth texture, indicating a relatively quiescent star formation history. There is a subtle blue tint to the outer regions of the galaxy, hinting at the presence of a younger stellar population compared to the bulge. The overall color profile suggests moderate dust content and ongoing, albeit subdued, star formation activity within the galaxy. There appears to be a slight asymmetry, suggesting possible minor gravitational disturbance or a past minor merger event. No prominent tidal features are observed.
