The galaxy presents a generally smooth morphology, exhibiting a dominant central bulge. The bulge appears largely featureless and is surrounded by a fainter, more diffuse halo that is only marginally resolved. The galaxy exhibits a slight ellipticity, deviating only minimally from a perfectly circular shape. There's no strong evidence of spiral arm structure or prominent dust lanes within the image resolution. Faint irregularities are detected on its outer edges, suggesting that it is not entirely undisturbed, but shows little evidence of major mergers or tidal interactions. The color profile appears somewhat homogenous with a slightly bluer central region, which implies some modest amount of ongoing star formation, although at a low rate.
