The galaxy presents as a lenticular or possibly an elliptical type, exhibiting a smooth, centrally concentrated luminosity profile. The core region appears bright and slightly yellow-tinted, suggesting a population of older stars and potentially a significant bulge component. Moving outward from the center, the light gradually fades. The overall shape is elongated, approaching a cigar-like morphology, indicating a lack of strong spiral arm structures. There is faint blue light concentrated at the outer edges of the galaxy, indicating the presence of some recent star formation, though the central core dominates. No prominent dust lanes or active galactic nucleus features are immediately apparent. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger events or tidal distortions.
