This galaxy appears to be an elliptical type, characterized by a smooth, featureless light distribution. It exhibits a generally round morphology, with a slight elongation along one axis, giving it an in-between, though not perfectly spherical appearance. There is no visible evidence of spiral arms or a prominent disk structure. The galaxy appears to be relatively isolated, with no signs of a major ongoing merger or significant tidal disturbances. The core of the galaxy exhibits a high surface brightness, suggesting a concentrated population of stars. The overall color profile indicates a population dominated by older stars, with a lack of significant ongoing star formation. The galaxy exhibits a redder color, indicating older stars.
