The galaxy presents as a centrally concentrated object with a smooth, somewhat elliptical morphology. It exhibits a dominant central bulge, appearing more luminous and densely packed than the surrounding galactic structure. The color profile suggests a likely evolved stellar population, skewed towards the redder end of the spectrum. While the central region dominates the light output, there are hints of extended, fainter features around the core, perhaps indicating a disk or halo component. There appear to be no obvious spiral arm structures or dust lanes visible in this image. There appears to be a second region of concentrated mass, which may indicate that this is a galaxy interacting with a companion galaxy. This disturbance makes it likely that the galaxy is not relaxed and might be in the process of merging. 
