The galaxy presents a generally smooth morphology, with a centrally concentrated light profile. It exhibits a relatively elliptical shape, appearing moderately rounded rather than highly elongated. The galaxy displays a yellowish hue, indicative of an older stellar population and a lack of significant ongoing star formation. There is a suggestion of some minor disturbance in the galaxy's structure, potentially due to past interactions or internal dynamics. A secondary, nearby object is present, possibly indicating a minor merger or close interaction. The galaxy is relatively large, suggesting it is a massive system.
