The galaxy presents as a smooth, elliptical-like structure with a distinct cigar shape. The central region exhibits a concentrated brightness, indicating a significant stellar density, possibly an active galactic nucleus or a dense nuclear star cluster. The color profile is dominated by redder hues. The light gradually fades towards the outer edges with little visible dust or gas lanes. There are no spiral arms or bar-like features detected. The galaxy is not currently undergoing any major merging activity. It has a high likelihood of not being disturbed, and not actively merging with any other object.
