The galaxy presents as a disk galaxy, viewed at a moderate inclination. Its morphology is generally smooth, exhibiting an elliptical profile, tending toward a cigar shape. A noticeable central bulge is present, with a redder hue, suggesting a population of older stars. The disk component appears bluer, consistent with the presence of younger stellar populations and active star formation. The disk structure shows some irregularity, possibly indicating minor disturbances or ongoing interactions. There is no clear evidence of major merging activity. Overall, the galaxy appears as a well-defined system with a significant stellar mass.
