The galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated with a mostly circular shape. There is some indication of slight asymmetry in the overall distribution of light, with a possible extension or plume visible on one side. The galaxy exhibits a color gradient, appearing bluer in its central region and trending towards redder hues in its outer portions. This color gradient is consistent with a centrally concentrated population of younger, bluer stars and an older, redder stellar population in the outer regions. There is no strong indication of prominent spiral arms or a well-defined disk structure. The galaxy appears to be relatively isolated, without obvious signs of tidal interactions or ongoing major mergers in this particular image.
