The galaxy presents a mostly smooth morphology with a hint of disk-like structure. It appears to be a relatively massive system with a substantial population of older stars, giving it a redder color. The galaxy is more elliptical than spiral and has a relatively compact appearance. There is no prominent spiral arm structure or central bar visible. The light distribution is centrally concentrated with a gradual decline in brightness towards the outer regions. No significant tidal features or signs of recent major merger activity are apparent, although there might be evidence of a minor disturbance or interaction given its slightly irregular shape.
