The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that appears yellow-white in color, suggesting an older stellar population. The surrounding disk component is less pronounced, exhibiting a gradual fading outwards from the core. It is elongated, and there is no strong evidence of spiral arm structure or prominent dust lanes. A faint, diffuse extension is visible on one side, potentially indicating a minor tidal disturbance or interaction. Overall, the galaxy's morphology appears largely undisturbed, with no signs of major merging activity.
