The galaxy presents an overall elliptical morphology, appearing somewhat compact. The central region exhibits a brighter, more concentrated luminosity profile, with a smooth transition toward the outer edges. There is evidence of a faint, extended halo or disk structure surrounding the central core. The color gradient suggests potential stellar population differences within the galaxy. The core region is composed of blue stars, and toward the outer edges, the hue changes, indicating older stars or the presence of dust. The galaxy does not display any prominent spiral arm structures. There also seems to be a tidal tail or some sort of dust in the lower left corner of the galaxy, which seems to be causing a disturbance. There is no clear indication of a major ongoing merger event, although a slight distortion or irregularity in the outer structure may suggest minor interaction. The galaxy's overall smooth appearance suggests it is either an elliptical galaxy or a relatively face-on disk galaxy with a dominant bulge.
