The galaxy presents as an elliptical structure, elongated along a discernible major axis. The central region exhibits a bright, concentrated luminosity, indicative of a substantial stellar population and potential central supermassive black hole activity. The overall color profile suggests a mix of stellar populations, with a yellowish hue in the core possibly corresponding to older, redder stars. Moving outwards from the core, there is a subtle shift towards bluer tones. This may indicate the presence of younger, hotter stars in the outer regions, though the limited resolution makes definitive classification of stellar populations challenging. The outer regions are less defined, exhibiting a gradual decrease in surface brightness. There's a slight asymmetry that could suggest minor tidal interactions.
