This galaxy appears to be a relatively compact object with a dominant, bright central region exhibiting a smooth, albeit slightly irregular, distribution of light. The overall shape is somewhat amorphous, lacking a clear spiral structure or defined elliptical form. There is evidence of subtle disturbances or irregularities in the outer regions of the galaxy, possibly indicative of tidal interactions or past minor merger events. The color profile suggests a significant population of older stars, with a possible hint of bluer, younger stars in the central area indicating ongoing or recent star formation in this region. There is a slight asymmetry in the distribution of light, potentially suggestive of a minor disturbance in the overall structure. Overall, the galaxy exhibits characteristics somewhere between a relatively smooth elliptical and a perturbed disk galaxy.
