The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. Its light distribution is relatively smooth, suggesting a lack of significant spiral arm structures. The color profile indicates a dominance of older stellar populations, emitting primarily in the redder wavelengths, which is consistent with a relatively low star formation rate. There is a possible small interacting object to the right of the primary galaxy. There appears to be minimal evidence of strong tidal disturbances or ongoing merger activity. Overall, it appears to be a quiescent elliptical galaxy.
