This galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. It exhibits a predominantly yellow-orange hue, indicative of an older stellar population and a relative lack of ongoing star formation. The galaxy appears to be relatively isolated, displaying no obvious signs of major tidal disturbances or ongoing mergers. The shape is consistent with a slightly elongated spheroid. The absence of distinct spiral arms or a prominent disk structure suggests a classification towards the earlier end of the Hubble sequence.
