The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. Its overall shape appears elongated, with a noticeable deviation from a perfect circle. There is no obvious spiral arm structure or prominent dust lanes visible. The color profile suggests a more evolved stellar population, leaning towards redder hues. The galaxy appears to be relatively isolated, with no obvious signs of major interactions or merging events. It possesses a concentrated core with gradually diminishing luminosity towards its outer regions, giving the impression of a galaxy with a relatively stable and mature configuration.
