The galaxy presents a lenticular morphology, appearing as a flattened ellipse in the image. Its central region exhibits a concentrated, yellowish-white luminosity, suggestive of an older stellar population. The outer regions of the galaxy display a bluer hue, possibly indicative of ongoing star formation, although this activity appears subdued. The galaxy appears relatively smooth, with no obvious spiral arm structures or major dust lanes visible. A slight asymmetry in the outer regions hints at a possible minor interaction or past disturbance. The overall form of the galaxy is elongated, displaying a notable cigar shape. There are no apparent signs of major merging activity.
