The galaxy appears to be an elliptical galaxy, based on its smooth light distribution and lack of spiral arm structures. It presents a centrally concentrated luminosity profile, with the brightest region located at the core. The shape is elongated, approximating a cigar shape, suggesting a moderate degree of ellipticity. The color is predominantly yellowish, indicating a stellar population dominated by older, redder stars and a relatively low rate of ongoing star formation. There is no apparent evidence of recent or ongoing mergers, although a faint disturbance cannot be ruled out due to the image resolution.
