The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a centrally concentrated luminosity profile. The overall color is yellowish-white, suggesting an older stellar population with a lower rate of ongoing star formation. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy is mostly rounded in shape, showing some signs of being slightly off-center. There are indications of a minor disturbance, possibly due to a small tidal interaction or minor merger event in its past, though it is not currently undergoing a major merging process.
