The galaxy presents a morphology suggestive of an elliptical type, characterized by a relatively smooth, centrally concentrated light distribution. The core region exhibits a brighter, more intense yellowish hue, indicative of an older stellar population. The overall shape appears somewhat elongated, but generally round. There is a suggestion of a slight asymmetry in the outer regions. The color gradient transitions from yellowish in the core to a somewhat bluer tinge in the surrounding regions. This may indicate regions of more recent, although limited, star formation activity towards the outskirts of the galaxy. No clear spiral arms or distinct features, such as dust lanes or prominent star clusters, are apparent. Overall, the galaxy appears to be a fairly well-formed elliptical galaxy with potentially subdued star formation activity.
