The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It is likely an elliptical galaxy, or possibly a lenticular galaxy viewed at a low inclination. The galaxy exhibits an elongated shape, with a somewhat cigar-shaped appearance. The colour profile suggests an older stellar population with a yellowish hue. This is consistent with a relatively low ongoing star formation rate, indicating most of the star formation occurred at some time in the past. There appear to be some minor disturbances, suggesting a possibility of a past minor merger event. No spiral arms are visible. Based on the estimated size, the galaxy appears to be of moderate physical extent.
