This galaxy appears as a relatively compact object with a bright, concentrated core. There is a degree of fuzziness surrounding the central region, hinting at a possible extended halo or envelope of stars. The color profile suggests the presence of both older stellar populations, indicated by the redder hues, and some younger, bluer populations closer to the central region. The galaxy exhibits some signs of minor disturbances, with a slight asymmetry visible in the outer regions. There is a hint of possible tidal features, although these are subtle. The overall morphology could potentially be classified as an early-type spiral or a lenticular galaxy with a significant bulge component. There's also the possibility of a past or ongoing minor merger event contributing to its disturbed appearance.
