The galaxy presents as a largely featureless, elliptical-like structure with a smooth, concentrated luminosity profile. Its core is significantly brighter and exhibits a yellowish-white hue, suggesting a population of older stars and a possible lack of significant ongoing star formation in that region. The galaxy fades gradually towards its outer edges, presenting a less concentrated, dimmer halo. The faint greenish-blue tint in the extended areas around the core may suggest that the galaxy does have some star formation, or a faint disc, but it isn't particularly pronounced. There are no obvious spiral arm structures or dust lanes visible, indicating a morphology that is likely dominated by an evolved stellar population. The overall shape appears approximately round, lacking any significant elongation or asymmetry that would indicate a recent merger event, or a particularly barred spiral.
