The galaxy presents a somewhat elongated, cigar-shaped morphology. It exhibits a smooth, diffuse light distribution, with a noticeable central concentration but no clearly defined spiral arms or bar structure. There may be some very subtle disturbances visible on the edges of the galaxy but it seems to be primarily undisturbed.

Color gradients are present, with a slightly bluer hue on the edges and a redder hue towards the center, potentially indicating ongoing or recent star formation activity towards the galactic edges, and/or an older stellar population dominating the central bulge. The galaxy appears to be relatively isolated, with no immediate signs of strong tidal interactions with nearby galaxies.
