The galaxy appears as a roughly elliptical, compact object with a bright central core. There is a slight elongation, but the overall morphology suggests a relatively featureless spheroid. A faint, diffuse halo surrounds the bright core, extending outwards but fading rapidly with distance. There is little evidence of spiral arm structure or a prominent disk. Color analysis shows a stronger presence of light in the redder bands, with a moderate presence of the blue band, although dominated by the green. This suggests an older stellar population and relatively low ongoing star formation. There are slight irregularities to the galaxy's shape, particularly in the faint outer regions. These could indicate minor tidal disturbances or interaction with smaller neighboring galaxies, but the signal is not strong. No evidence of a major merger is present, but this cannot be ruled out.
