The galaxy presents as an elliptical morphology, displaying a smooth, though somewhat elongated, light distribution. The central region exhibits a higher concentration of luminosity, appearing as a bright, yellowish core, suggestive of an older stellar population. The outer regions of the galaxy fade gradually into the background sky, with only subtle color variations noted across the galactic body. There is minimal evidence of distinct spiral arm structure, star-forming regions, or prominent dust lanes. Overall, the galaxy seems to be in a relatively quiescent state, with potentially low star formation rates. There does not appear to be any evidence of a major merger event or significant tidal disturbance.
