The galaxy presents as a central, luminous bulge surrounded by a fainter, more diffuse disk. The color gradient transitions from a bright, yellowish core, suggestive of an older stellar population dominated by red giant stars, to a bluer periphery indicative of more recent star formation activity. The morphology appears generally smooth with hints of discal features but lacking well-defined spiral arms or bar structures. There is no obvious evidence of a major ongoing merger or significant tidal disruption. Subtle irregularities in the outer disk may indicate minor gravitational interactions or internal processes influencing the galactic structure. The overall shape approximates an elliptical galaxy with a notable flattened component.
