The galaxy presents a generally elliptical morphology, appearing mostly smooth with a high degree of central concentration. A dominant, bright central bulge exhibits a yellowish hue, suggesting a population of older, redder stars. Fainter, bluer light is visible in the outer regions, possibly indicating some ongoing star formation. There appears to be little in the way of spiral arm structures and the galaxy is not experiencing a major merger. There are also slight asymmetric features near the lower central part of the galaxy. Overall, the galaxy appears to be relatively isolated, not displaying any prominent tidal distortions or interactions with neighboring galaxies, and has a substantial mass.