The galaxy presents as a roughly elliptical structure, elongated along its major axis, with a cigar-like shape. The light distribution appears smoother and more concentrated toward the galactic center. The central region exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. Moving outward from the center, the galaxy gradually fades into the background. Faint hints of reddish tones are present in the outer regions, potentially indicating the presence of dust lanes or regions of ongoing, albeit low-level, star formation. Overall, the galaxy lacks distinct spiral arms or prominent features, characteristic of a relatively smooth morphology. There are no significant signs of any recent major merger events, such as tidal tails or highly disturbed morphology, though there could be some minor disturbance present.
