The galaxy appears to be a relatively compact object. Its morphology suggests a predominantly smooth structure. The core region displays a concentrated luminosity, with a gradual falloff in brightness towards the outer edges. Color gradients are subtle but present; the central area seems slightly more yellow, possibly indicating an older stellar population, while the outer regions show a bluer tint, which may be due to the presence of younger, hotter stars.

The overall shape appears somewhat elliptical, although there is a deviation from perfect roundness. There might be subtle irregularities or minor disturbances in the outer regions, but without further data, it is difficult to ascertain the cause. There is no definitive evidence of a major ongoing merger, or a significant tidal interaction with another galaxy.
