The galaxy appears as a moderately bright, relatively compact object. It is somewhat elliptical in shape, displaying a smooth, diffuse light distribution with a concentrated central bulge. The overall color suggests an older stellar population, with a yellowish-red hue indicating a lack of significant ongoing star formation. The galaxy does not exhibit well-defined spiral arms or any prominent dust lanes. There is some evidence of possible minor disturbances in the galaxy's structure, potentially indicating a past or ongoing interaction or merger. The absence of clear tidal tails or other major distortions suggests that the interaction, if present, is not exceptionally violent or recent. 
