The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a moderate degree of roundness in its overall shape, with a minor deviation towards a more elongated form. There's little evidence of spiral arms or prominent disk features. The light distribution appears fairly even, lacking the concentrated central bulge and disk observed in spiral galaxies. The primary color appears to be yellowish white with red tinges, suggesting an older stellar population, and low active star formation rate. There are no visible tidal tails or other signs of major recent merging activity or significant galactic disruption. However, there are some very minor disturbances in the edge of the object that may suggest some minor merger activity in the past.
