The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its overall shape appears elliptical, elongated along one axis. The color profile indicates a population dominated by older stars, displaying a yellowish to reddish hue concentrated towards the center. The edges of the galaxy gradually fade into the background sky, indicating a diffuse halo. There is minimal evidence of spiral arm structure or dust lanes within the visible portion of the galaxy. There are very faint, subtle hints of a disk-like structure, but the galaxy is largely dominated by a spheroidal component. The galaxy does not appear to be undergoing any major merging events. Slight disturbances or minor interactions, if present, are subtle and do not dramatically distort the overall structure.
