The galaxy presents a generally smooth morphology, with a high degree of central concentration. The central region exhibits a bright, somewhat diffuse bulge, suggestive of an older stellar population. There is faint, somewhat mottled structure that may suggest a minor disturbance within the disk of the galaxy. There is a noticeable slight extension or distortion of the galaxy's structure. There are no clearly defined spiral arms visible. The overall shape is somewhat rounded with a slight deviation toward an elliptical form. The color distribution suggests a redder central region, possibly indicating older stars and/or a higher concentration of dust, with a shift toward slightly bluer hues in the outer regions.
