The galaxy presents a largely featureless, smooth appearance, with a concentrated central bulge that fades gradually outward. The overall shape is generally round. There is no obvious spiral structure, bar, or signs of recent major merging events. A slight blue tint is observable at the outer edges suggesting some, though relatively low, level of star formation activity. The galaxy appears relatively compact. The light profile suggests a well-established stellar population, indicative of an older system with lower specific star formation rate.
