The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge that fades gradually into an extended halo. The color gradient suggests a population of older stars dominating its composition. A subtle disk-like structure may be present, but it is not well-defined, implying that the galaxy is dominated by random stellar orbits. There is a hint of a minor disturbance, perhaps from a small past interaction, though there is no clear evidence of a major ongoing merger. The galaxy appears to be relatively isolated, lacking significant signs of tidal features or companions. A small red structure is present on the edge of the galaxy. Given the smooth morphology and older stellar population, this is likely an early-type galaxy with a relatively low rate of star formation.
