The galaxy presents as a slightly elliptical, lenticular form. Its central bulge appears luminous and concentrated, displaying a yellowish-white hue, possibly indicative of an older stellar population. There is a smooth transition in luminosity from the core outward, with the extended disc exhibiting a fainter, more diffuse glow. No distinct spiral arm structures or prominent dust lanes are discernible within the resolution of this image. There is very little indication of ongoing star formation, which agrees with its high level of smoothness. There may be some minor disturbances.
