The galaxy presents a generally smooth appearance, though subtle features suggest a more complex structure. It exhibits a slightly elliptical shape, with a central bulge that appears relatively bright and concentrated. Extending from the central region are faint, diffuse arms or extensions, hinting at a possible disk-like component, although distinct spiral arms are not readily apparent. The overall color profile appears somewhat blueish, potentially indicating the presence of younger stellar populations and ongoing, albeit low, star formation. The outer regions of the galaxy fade gradually, lacking a sharp boundary and suggesting a relatively extended halo or envelope of stars. There are slight disturbances in the structure that may be evidence of a minor merger. There is a significant amount of light coming from this galaxy despite its relatively smooth features.
