The galaxy presents a roughly elliptical morphology, with a high degree of central concentration. The light profile appears smooth, with little evidence of spiral arm structure or significant dust lanes. The dominant color is yellow-orange, suggesting an older stellar population. A distinct blue region appears offset from the galactic center, perhaps indicative of a region of on-going star formation. The overall morphology suggests that the galaxy is not currently undergoing a major merger, though some tidal interaction is not entirely excluded. The system is compact, indicating a relatively small size, although distance effects could influence this observed size.
