The galaxy appears to be an elliptical or lenticular type, with a smooth, largely featureless morphology. The central region is bright, with a concentrated luminosity profile suggesting a significant stellar population. A slight color gradient is visible, with the core appearing more yellow/red and the outer regions showing hints of green/blue. This could be due to an older stellar population in the core and some ongoing, but minimal, star formation in the outer regions, though dust extinction could also play a role. There is no apparent spiral structure, bar, or other significant morphological disturbance indicating that it is a relatively undisturbed system and likely not undergoing major merging activity. The galaxy appears to be isolated, with no obvious tidal tails or interactions with nearby companions. Its shape is nearly circular, with no signs of strong elongation or asymmetry. Overall, the galaxy appears as a mature, quiescent system with relatively low star-formation activity and no major recent interactions.
