The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light distribution suggests a fairly uniform stellar population. The galaxy's overall shape is generally round, with no obvious signs of a prominent disk structure or strong tidal disturbances. There is a subtle color gradient, with the central region appearing slightly yellower than the outer halo, suggesting a possible difference in stellar populations or dust content between the core and outer regions. There is very little evidence of active star formation, given the lack of blue light, prominent spiral arms, or irregular features. The galaxy appears undisturbed, with no signs of recent or ongoing major mergers.
