The galaxy presents an overall elliptical morphology, appearing somewhat cigar-shaped. Its central region exhibits a bright, concentrated core suggesting a high stellar density and potentially the presence of an active galactic nucleus. Moving outward from the core, the galaxy displays a smooth, diffuse structure, with a gradual decline in luminosity. There is faint evidence of some subtle features or disturbances in the outer regions, such as an uneven texture or slight asymmetry, which indicates possible minor interactions or past mergers. The color profile shows a predominantly yellowish-red hue, indicative of an older stellar population with lower rates of recent star formation.
