The galaxy presents an elliptical morphology, though some disk-like features are present. It shows a central bulge, which appears quite prominent and exhibits a yellowish hue, likely indicative of an older stellar population. The outer regions appear bluer, possibly suggesting ongoing or recent star formation. While mostly undisturbed, the galaxy's structure isn't perfectly smooth, hinting at minor internal disturbances or past interactions. No significant merger activity is immediately apparent, and the galaxy appears largely isolated.
