The galaxy appears to be a relatively smooth, elliptical type with a concentrated central bulge. It exhibits a high degree of roundness, with no apparent bar structure or spiral arms. The galaxy's light profile is smooth and decreases radially from the center.

There is no evidence of significant tidal features, strong dust lanes, or ongoing mergers. Based on the color, the galaxy appears to be composed of an older stellar population, with a moderate degree of star formation. The overall morphology suggests a galaxy that has undergone a period of quiescence and is not currently experiencing major starburst activity.
