The galaxy appears to be an elliptical type. It exhibits a smooth, symmetrical morphology with a concentrated central bulge. There is no discernable spiral arm structure or dust lane. The color profile suggests a stellar population dominated by older, redder stars, with a hint of bluer stars possibly indicating some ongoing star formation. The galaxy exhibits an overall round appearance, with some asymmetry. There is no evidence of tidal disturbances or a recent major merger event. The galaxy has a moderate amount of star formation.