The galaxy presents as a disk galaxy, viewed nearly edge-on from our vantage point. The prominent central bulge appears smooth and somewhat elongated along the disk's axis. The bulge exhibits a concentration of light intensity towards its core, suggesting a high density of stars within that region. Extending outwards from the bulge, a relatively faint and thin disk structure can be observed. The disk shows some indication of obscuring dust lanes, but it is mostly smooth and lacking in distinct spiral arm features, as this galaxy has likely exhausted most of its gas supply. There is no strong evidence of ongoing major merger activity, although there are some slight indications of a minor gravitational disturbance in the disk. The galaxy's overall color suggests a population of older stars.
