The galaxy presents as a relatively smooth, elongated structure. Its light is dominated by a bluish-white hue, indicating the presence of younger, hotter stars, although there may be some faint reddish tones indicative of older stars. The lack of defined spiral arms or a prominent bulge suggests it is likely a lenticular or possibly an elliptical galaxy. The smooth light distribution indicates no major ongoing mergers, although some minor disturbances cannot be ruled out due to the slightly irregular shape. No dust lanes or other indicators of significant gas content are apparent in the image. Overall, the galaxy appears to be relatively quiescent, with a moderate level of star formation. The shape of the galaxy is more similar to a cigar than a circle.
