The galaxy presents as a moderately compact, elliptical structure. Its overall shape is generally smooth and appears undisturbed, lacking prominent spiral arms or significant morphological irregularities. The light distribution is centrally concentrated, with a gradual decline in luminosity extending outwards from the core.

The color profile indicates a tendency toward redder hues, which may suggest an older stellar population and a lower rate of ongoing star formation. However, there's also a subtle blue component present, indicative of some level of recent or ongoing star formation.
