The galaxy presents a predominantly smooth morphology, with little evidence of spiral arm structure or pronounced dust lanes. It exhibits an elliptical shape, appearing mostly symmetrical. The central region displays a bright, concentrated core which fades gradually outward. The overall color profile suggests a population of older stars, as indicated by the yellowish hue, which could possibly indicate low star formation. There appears to be little to no ongoing major merging activity, though there may be evidence of minor tidal disturbance in the outer regions. The estimated size suggests a moderate physical extent.
