The galaxy appears to be an elliptical type, displaying a smooth, featureless morphology. The shape is elongated, with a cigar-like appearance. Color gradients are visible, with the central region exhibiting a yellowish hue that may indicate a higher concentration of older stars. The outer regions show a bluer tint, potentially suggesting the presence of younger stellar populations or ongoing star formation activity. No signs of strong gravitational disturbance, such as tidal tails or merging features, are apparent in the immediate vicinity of the galaxy. The observed structure appears relatively stable.
