The galaxy presents as a somewhat elongated, disk-like structure, consistent with a possible spiral or lenticular morphology. It exhibits a prominent central bulge, appearing yellowish-white in color, which likely indicates a higher concentration of older stellar populations. Extending outward from the bulge, fainter, bluish regions are visible. These areas suggest the presence of younger, hotter stars and ongoing star formation. The disk appears relatively smooth, with no distinct spiral arm structures readily apparent in this image. There might be some minor disturbances, but the overall structure looks to be relatively unperturbed. The galaxy's color profile, shifting from yellowish in the center to bluish at the edges, reinforces the expectation of varying stellar populations and activity levels across its structure. It has a low chance of being a merger event. The overall shape could be described more as cigar shaped.
