The galaxy appears to be an elliptical type, characterized by a smooth, largely featureless morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The overall shape is nearly circular, showing minimal deviation from a spheroidal form. The galaxy displays a color gradient, with a yellowish-orange core transitioning to slightly redder hues in the outer regions. This suggests an older stellar population dominating the central region. There is no evidence of prominent spiral arms, dust lanes, or ongoing major merging activity. Minor disturbances cannot be ruled out, though they would appear to be subtle and not drastically impacting the overall structure. The relative smoothness and roundness, alongside the redder color profile, are consistent with a galaxy where star formation has largely subsided, leaving behind a population of aging stars.
