The galaxy presents as a relatively diffuse, centrally concentrated structure. It appears somewhat elliptical, but with some subtle irregularities in its overall shape, particularly at the edges. The color profile shows a general trend from slightly bluer hues in the central area, transitioning to redder tones toward the outer regions. There is some indication of faint, extended tidal features. The image suggests there could be evidence of past or ongoing gravitational interactions. The central region of the galaxy appears smooth and featureless, with no obvious spiral arm structures or prominent dust lanes. This suggests the galaxy may be an early-type spiral or a lenticular galaxy.
