This galaxy exhibits a generally smooth morphology with a hint of a disk-like structure. The shape is elongated, appearing cigar-shaped. There is a concentrated central bulge of yellowish light, possibly indicative of an older stellar population. The outer regions of the galaxy display a bluer hue suggesting the presence of younger, hotter stars, albeit not in distinctly resolved spiral arms. There is no significant evidence of major ongoing mergers, though there is a slight asymmetry on the left side of the galaxy, suggesting possible minor interaction or internal disturbances. The overall appearance suggests an intermediate galaxy, possibly a lenticular (S0) or early-type spiral galaxy viewed at an oblique angle.
