The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region, with light intensity gradually decreasing outwards. There is no prominent disk structure or spiral arm features visible. The overall color appears to be a yellowish-white, suggesting a population of older stars and a relatively low rate of on-going star formation. There might be a very faint, diffuse halo extending beyond the main body of the galaxy. No signs of any major mergers or tidal disturbances are immediately apparent. The galaxy appears to be well-defined and relatively isolated.
