The galaxy presents as a relatively smooth, elliptical-like structure, with a color profile that suggests it consists of an older stellar population, based on the strong red color. It does not exhibit a prominent spiral arm structure or a well-defined disk, which supports the smooth classification. The light is centrally concentrated, with a gradual decrease in intensity towards the outer regions. There may be a faint indication of a tidal feature, although the image resolution limits a full assessment. No dust lanes are clearly visible across the galaxy's face.
