The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. There is a lack of readily discernible spiral arm structure or prominent dust lanes. The overall shape appears roughly elliptical or circular. The light distribution suggests a relatively uniform stellar population, exhibiting a color profile that transitions gradually from a brighter, possibly older, population in the core to a fainter, slightly bluer, population in the outer regions. Subtle irregularities in the outer regions may indicate minor tidal disturbances or interactions, but these features are not prominent. The galaxy exhibits a noticeable degree of roundness, with no significant elongation or bar structure visible. There is no obvious indication of ongoing major mergers or significant starburst activity based on the overall color and morphology.
