The galaxy presents a largely smooth and somewhat elliptical morphology. It exhibits a subtle elongation, trending towards a cigar-like shape. No prominent spiral arms or distinct bar structures are discernible. The light distribution is concentrated towards the center, suggesting a prominent bulge. Color gradients are subtle, with a slight reddening towards the galactic core and subtly bluer outer regions. This could indicate a population of older stars in the central bulge, and younger, hotter stars in the outer regions, respectively. Overall, the galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal distortions. There might be a very minor disturbance. The galaxy appears to be in a relatively quiescent state regarding star formation.
