The galaxy presents as a pair of interacting galaxies. The larger component exhibits a smooth, elliptical morphology. It displays a concentrated central bulge with a diffuse halo, suggesting a relatively old stellar population. Its color is yellowish, indicative of older stars dominating the light output. There is little evidence of significant ongoing star formation within this galaxy.

The smaller component shows a more disturbed structure. It is more compact than the larger galaxy and exhibits a bluer color. The irregular shape and blue color indicate the presence of younger stars and ongoing star formation. Evident tidal features suggest gravitational interaction between the two components. There appears to be a faint bridge of material connecting the galaxies, signifying a possible ongoing merging process.
