The galaxy presents a lenticular morphology, displaying a smooth, disk-like structure with a prominent central bulge. It has a relatively high degree of ellipticity. The light distribution suggests a more cigar like morphology when compared to a perfectly round morphology. The overall color profile is characterized by a bluer hue in the disk region with the central bulge exhibiting a yellowish hue. There is no strong evidence of spiral arm structure or significant dust lanes visible at this resolution. The galaxy does not show any strong indications of major mergers or tidal disturbances. The overall appearance suggests a passively evolving system, with intermediate mass.
