The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The central region exhibits a concentrated, bright core, suggesting a higher density of stars. A subtle color gradient is observed, with the core appearing more yellow/orange, possibly indicating an older stellar population and a lack of significant ongoing star formation in the nucleus. Moving outward from the core, the galaxy exhibits a faint, diffuse halo, showing a slight blue tinge in some areas. This may represent the presence of younger stars, though in relatively small numbers. The overall shape is somewhat elongated, deviating slightly from a perfectly circular profile. There is no evidence of spiral arms, bars, or prominent dust lanes. The galaxy appears to be relatively isolated, showing no obvious signs of interaction with other galaxies.
