The galaxy presents a largely smooth and concentrated appearance, suggesting an elliptical morphology. The central region exhibits a bright, yellowish hue, indicative of an older stellar population dominating the core. There is limited evidence of a disk structure or spiral arms. Some faint blue tinges on the outer edges could indicate a low level of on-going star formation in these regions, although this is minimal. Overall, the galaxy presents a relatively quiescent and evolved state, with an intermediate mass. There are no apparent signs of any major mergers or tidal disturbances. The galaxy is round in shape, with no major visible asymmetry.
