The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity outward from the core. There is a suggestion of slight elongation, but the overall shape approximates a spheroid. The color is generally yellowish, with hints of red, indicative of an older stellar population and reduced ongoing star formation. A possible merger or tidal interaction may be occurring, as indicated by the presence of a neighboring bright spot, though higher resolution imaging would be necessary to determine this definitively. No prominent dust lanes or spiral arm structures are discernible in the image.
