The galaxy appears to be a relatively smooth, elliptical system. The central region exhibits a yellowish hue, suggestive of an older stellar population, while the outer edges transition to a bluish color, potentially indicating the presence of younger, hotter stars. The galaxy has a cigar-like shape. There is no visual evidence of any major disturbances, such as tidal tails or strong asymmetries, that would indicate a recent major merger event. Faint, diffuse light extends from the central body, gradually fading into the background. No dust lanes or spiral arm structures are discernible in this image.
