The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth light distribution with a high degree of central concentration. The core region demonstrates a bright, intensely luminous profile, suggesting a dense stellar population and possibly an active galactic nucleus, although no distinct jet or accretion disk is visually apparent. The color index, assessed from the blended RGB image, indicates a bias toward redder wavelengths. There are no prominent dust lanes or spiral arm structures. A subtle extension along the major axis is discernable, but the overall shape is more closely aligned with a spheroidal geometry, with only a small level of asymmetry or disturbances. There is no evidence of a significant tidal interaction or recent merger event based on the morphology. The lack of blue star-forming regions implies a low rate of star formation.
