The galaxy presents as a relatively compact object with a slightly elongated morphology. It exhibits a smooth overall appearance, with some suggestion of faint disk-like features internally. The color profile shows a central concentration of redder hues, which suggests an older stellar population in the galactic bulge. Moving outward, the colors shift towards bluer tones, indicating the presence of younger, star-forming regions. There may be minor disturbances present in the overall structure. The galaxy exhibits characteristics associated with late stage merging activity.
