The galaxy presents a somewhat elliptical morphology, appearing elongated with a discernible cigar-shaped structure. A considerable fraction of the galaxy's light seems to be concentrated within a smooth, central bulge. There are areas of redder light emission within the galaxy, potentially indicative of areas of ongoing or past star formation. The overall color suggests a relatively evolved stellar population, with possible traces of younger stars. The galaxy does not display strong evidence of a major ongoing merger, though there is some hint of minor tidal disturbance in its morphology, suggesting potential gravitational interaction with a nearby galaxy.
