The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is somewhat elongated, resembling a cigar shape. There is little evidence of spiral arm structure or prominent features, suggesting a morphology leaning towards an elliptical galaxy, or possibly a lenticular galaxy viewed at an angle.

The light profile appears to be smooth, with the brightest region concentrated in the center and a gradual fall off in brightness further away from the core. The color gradient indicates a redder core, likely populated by older stars, that transitions to bluer hues at the outer edges, which could indicate more recent star formation is more active in these regions. No signs of any major disturbances or interactions with neighboring galaxies are visibly apparent. The galaxy appears to be relatively isolated and undisturbed.
