The galaxy presents a largely smooth morphology, with minimal discernible substructure or spiral arms. The light distribution appears centrally concentrated, suggesting a possible elliptical classification. The overall color profile exhibits a redder hue, indicative of an older stellar population and/or significant dust content. There is a slight elongation, as opposed to being perfectly circular, though it is only a minor deviation. A possible minor disturbance or faint tidal feature is present in the lower right quadrant. This may imply a past or ongoing interaction with another galaxy. Overall, the galaxy appears relatively undisturbed and mature. The low star formation rate supports this.
