This galaxy presents as a slightly elongated, ellipsoidal structure. The central region exhibits a bright, concentrated core, suggesting a substantial stellar population. The overall color appears to be reddish-yellow, indicative of an older stellar population with a lower proportion of young, blue stars. Faint extensions of light are visible extending from the central region, potentially suggesting a disk-like structure or tidal arms from a minor disturbance. The galaxy displays a relatively smooth appearance, with no obvious dust lanes or prominent spiral arm structures. The galaxy is generally isolated, with no immediate indications of ongoing major merger activity.
