The galaxy presents as a moderately sized, elliptical-like structure. It exhibits a smooth, centrally concentrated light profile, with the intensity decreasing gradually from the core outwards. The central region shows a yellowish hue, suggesting the presence of an older stellar population. Moving outwards from the core, the color shifts towards a bluer tone, hinting at younger stars in the outer regions. The galaxy appears elongated with a noticeable major axis, displaying an apparent flattening. There are no obvious spiral arms or significant dust lanes visible. Overall, the galaxy appears relatively undisturbed, lacking prominent signs of recent merger activity or strong tidal interactions.
