This galaxy appears to be an elliptical type, based on its overall morphology. It exhibits a relatively smooth, featureless structure with a high degree of central concentration. The light distribution gradually decreases from the core outwards, indicating a centrally dominant stellar population. The galaxy is approximately round in shape, with a slight elongation that may suggest a mild departure from perfect sphericity. The colors appear to be relatively homogenous across the galaxy, suggesting a lack of significant ongoing star formation or prominent dust lanes. The overall color profile suggests a predominantly older stellar population. There is no obvious evidence of tidal features, mergers, or other significant disturbances in its immediate vicinity, hinting at a state of relative isolation. The galaxy does not display a prominent disk structure or spiral arms.
