This galaxy appears to be a relatively compact object, generally elliptical in shape. The central region exhibits a high degree of luminosity, suggesting a concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. Moving outwards from the core, the galaxy displays a fainter, more diffuse halo. 

There appears to be a slight asymmetry in the outer regions, with some distortion noticeable on one side, hinting at a possible gravitational interaction or past merger event. The overall color profile suggests a mix of stellar populations, with a relatively even distribution of bluer and redder stars, although bluer light is dominant. There is little evidence of prominent spiral arms or distinct dust lanes. The galaxy appears to be fairly isolated.
