The galaxy presents a largely smooth, elliptical morphology. A concentrated central bulge dominates the structure, exhibiting a yellow-orange hue, suggesting an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. The galaxy has a noticeable, albeit subtle, color gradient, with the outer regions appearing slightly bluer than the core. The isophotes exhibit a generally round shape, although slight deviations are visible. I find no evidence of any major mergers. There may be evidence of minor disturbance to the galaxy but overall, it appears to be relatively undisturbed.
