The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears to be ellipsoidal in shape, suggesting a dynamically relaxed system. The galaxy's color profile indicates an older stellar population, exhibiting a yellowish-red hue characteristic of evolved stars. There are no prominent spiral arms or dust lanes visible. There is a slight asymmetry in the outer regions, hinting at the possibility of a past minor interaction, or ongoing accretion. The overall structure is dominated by the smooth stellar distribution of the bulge, with minimal evidence of active star formation.
