The galaxy presents as a somewhat elongated, elliptical-like object. Its central region is characterized by a bright, concentrated luminosity, suggesting a high density of stars and potentially an active galactic nucleus. Moving outward from the core, the luminosity decreases gradually, and the outer regions appear more diffuse and less structured.

The galaxy exhibits a smooth overall texture. There is no clear evidence of spiral arms, dust lanes, or significant star-forming regions within this imagery. The light profile shows an absence of patchy or irregular features. The observed color is predominantly yellowish-orange, which implies an older stellar population with lower levels of ongoing star formation.

The elongation of the galaxy gives it a somewhat cigar-like appearance. There is no indication of any recent or ongoing mergers with another galaxy or any strong tidal disturbances. It appears to be a relatively undisturbed, evolved galaxy.
