The galaxy presents an elliptical morphology, appearing elongated with a cigar-shaped structure. The central region exhibits a smooth, featureless quality, with a higher concentration of light that fades gradually towards the edges. There is a suggestion of a possible interaction or minor disturbance affecting the shape of the main body, evidenced by a smaller, somewhat separate concentration of light. Overall, the galaxy exhibits a redder color profile, potentially indicating an older stellar population and reduced ongoing star formation.
