The galaxy presents a generally elongated, cigar-shaped morphology. Its light distribution appears relatively smooth and concentrated towards the center, with the intensity gradient decreasing towards the outer regions. There is little evidence of significant spiral arm structures or pronounced features. The galaxy exhibits a color gradient, appearing more yellow/orange near the central bulge and subtly bluer in the outer regions, hinting at potential variations in stellar populations. The overall smooth appearance suggests the galaxy is likely an elliptical or lenticular galaxy, with a dominant population of older stars. There are no obvious signs of recent major mergers or tidal disturbances. The galaxy appears relatively isolated, with no clear companion galaxies in close proximity.