The galaxy presents as a generally smooth object, with a subtle elongation suggestive of an elliptical morphology. The color profile indicates a dominant population of older stars, particularly concentrated towards the central bulge, which displays a yellowish-red hue. Fainter blue colors are visible in the outskirts of the galaxy. These colors indicate the presence of a younger population of stars in the spiral arms. The galaxy appears to be relatively isolated, without evidence of ongoing major mergers or significant tidal disturbances, although there are some hints of minor asymmetry in its outer regions. The galaxy is not perfectly spherical, displaying an intermediate shape that leans towards being cigar-shaped.
