This galaxy presents as a relatively smooth, elliptical-like structure. There is a prominent central bulge that exhibits a bright, concentrated luminosity, suggesting a high density of stars within this region. The light appears to be more concentrated in the central core, with colors indicating possibly older stellar populations.

The galaxy is slightly elongated, displaying an aspect ratio that suggests it is not a perfect sphere, but rather somewhat cigar-shaped. The outer regions appear more diffuse and fainter, with a gradual fading in intensity moving away from the central bulge. There is no clear evidence of distinct spiral arms or a well-defined disk structure in this image. No obvious signs of any recent major merger events or significant tidal disturbances in the form of tails or distortions of the overall shape are immediately apparent.
