The galaxy presents as a centrally concentrated object. Its overall shape is elliptical, appearing relatively smooth with no distinct spiral arm structures discernible. The light profile appears somewhat diffuse, transitioning from a brighter, unresolved core to a fainter, more extended halo. The color gradient suggests a population of older stars, given the overall reddish hue. There may be minor disturbances evident in the outer regions of the galaxy, suggesting a possible interaction or past merger event. However, no significant tidal tails or bridges are observed. The galaxy has a relatively low star formation rate. Overall the galaxy seems relatively undisturbed.
