The galaxy presents a generally smooth morphology, with a dominant central bulge that appears largely spheroidal. The color profile suggests a population of older stars, evidenced by the yellowish-red hue concentrated in the central regions. There are faint traces of a disk component, though it is not well-defined, and the spiral arms, if present, are not clearly discernible. The outer regions appear somewhat diffuse, exhibiting a gradual decline in luminosity away from the core. There are no readily apparent signs of ongoing major mergers or significant tidal disturbances. The overall impression is that of a relatively evolved galaxy, possibly an early-type spiral or lenticular galaxy.
