The galaxy presents as a moderately bright, elliptical-like structure. A concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population dominating the core. Moving outward from the core, a gradual transition to a bluish-white color is observed, potentially indicative of more recent or ongoing star formation within the galaxy's extended disk. The overall form is generally smooth with some slight disturbances on the outskirts, displaying hints of a disk structure without any prominent spiral arms. The galaxy does not appear to be undergoing any major merging activity, though there are some possible signs of minor tidal disturbances.
