The galaxy presents as a slightly elongated, moderately luminous object. There is a suggestion of a central bulge, which appears to be slightly offset from the main body of the galaxy. Color gradients are subtle, with the bulge exhibiting a redder hue compared to the rest of the disk which is predominantly white-ish. The edges of the galaxy are diffuse. There is a high probability that the galaxy is currently experiencing a merger or tidal interaction due to the presence of morphological disturbances with a second object. The estimated size of the galaxy suggests a moderate physical extent.
