The galaxy presents as a relatively smooth, elliptical morphology with a dominant central bulge. There is a faint suggestion of a disk component, though it appears tightly wound. The color profile suggests an older stellar population, exhibiting a yellowish-red hue overall. No active star forming regions are readily apparent, indicating a likely low specific star formation rate. There is no evidence of any tidal disturbances or ongoing mergers, suggesting a relatively undisturbed evolutionary history.
