The galaxy presents as a relatively compact and smooth object, exhibiting a primarily elliptical morphology with a high degree of central concentration. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's light profile appears largely uniform, transitioning smoothly from a bright, slightly yellowish core to a fainter, diffuse outer region. There are no apparent signs of ongoing major merger activity, although the possibility of minor tidal interactions or disturbances cannot be entirely ruled out based on this image alone. Overall, this galaxy appears to be a quiescent, evolved system likely dominated by an older stellar population.
