The galaxy presents a largely smooth, elliptical morphology, appearing relatively round in shape. A concentrated, bright core dominates the galaxy's central region, exhibiting a yellowish hue, indicative of an older stellar population. This core gradually fades into a less luminous halo. Some faint bluish regions surrounding the core suggest the presence of younger stars and perhaps ongoing, albeit subdued, star formation within the galaxy. There is no obvious sign of any major merger activity or significant disturbance to the galaxy's overall structure. Overall, the galaxy appears to be a relatively quiescent system.
