The galaxy presents a generally smooth morphology, with a noticeable central bulge. It appears somewhat elongated, with a suggestion of a disk-like structure, however, it is not well defined. The color profile indicates a redder central region possibly indicating older stellar populations in the bulge, while the outer regions present bluer tones, which are indicative of younger, hotter stars. There are some subtle irregularities or disturbances observed, although not strongly suggestive of a major merger event. Overall, the galaxy appears to be in a relatively quiescent state.
