The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. The light distribution is dominated by a bright, yellowish core that gradually fades into the outer regions. The shape is elliptical, exhibiting an intermediate axial ratio that is neither perfectly circular nor highly elongated. There is some indication of subtle structural features, such as a faint disky component, oriented approximately horizontally relative to the image frame, though this is not definitive and could be an artifact. The color gradients are subtle, with the central region showing slightly redder hues, indicating a higher concentration of older stars. There is little evidence of ongoing major star formation, or signs of a recent merger or tidal interactions. Overall, the galaxy appears to be a relatively evolved system, characterized by a dominant bulge population.
