The galaxy presents as a relatively compact, elliptical-like structure. Its overall morphology appears smooth and largely featureless, with no obvious spiral arms or strong bars visible at this resolution. The galaxy exhibits a centrally concentrated brightness profile, with the luminosity decreasing gradually towards the outer regions. Color gradients are subtly present, with a slightly bluer hue in the central region transitioning to a redder hue in the outer regions. This may indicate a younger stellar population in the core compared to the outskirts. No significant signs of tidal disturbances, major mergers, or active galactic nuclei are immediately apparent. Based on the smooth structure and color profile, this galaxy is likely an evolved system with a significant population of older stars and a relatively low rate of current star formation.
