This galaxy presents as a relatively small, elliptical object. The central region exhibits a bright, yellowish core, which appears to be the most luminous component. This core is surrounded by a more diffuse, greenish halo. The halo suggests a fairly uniform distribution of older stars, although there may be a slight increase in density toward the central region. The edges of the galaxy exhibit a slight reddening. No spiral arms or distinct dust lanes are visible. The overall structure indicates a galaxy that is likely dominated by an older stellar population and lacks significant ongoing star formation. There may be very minor irregularities in the outer regions, possibly indicative of a past minor merger event, although the overall smoothness and lack of significant disturbances suggest that it has been relatively undisturbed in recent history.
