The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish hue, suggesting a high density of older stars and minimal ongoing star formation in that region. Moving outwards from the core, the galaxy's color gradually fades to a slightly bluer tint, implying the potential presence of a younger stellar population in the outer regions, or perhaps a lower metallicity. The overall shape is elongated, with the light appearing more diffuse and spread out along the major axis. There's no discernible evidence of spiral arms or a distinct disk structure. Minor disturbances are barely visible, suggesting the possibility of a past or ongoing interaction, but these are not significantly disrupting the galaxy's overall smooth form.
