The galaxy appears as a concentrated central bulge surrounded by a less defined disk. The object presents a yellowish-red hue, suggesting a population dominated by older stars and relatively low ongoing star formation. The galaxy's morphology seems predominantly smooth, although there may be subtle hints of disk-like features or minor disturbances. The overall shape leans towards round, with minimal elongation observed. There appears to be a hint of possible merging activity or tidal interactions, but the main body displays no obvious or major structural disruption. This object appears to be a massive system.
