The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is generally round, with no obvious signs of significant asymmetry or elongation. The light distribution appears largely homogenous. There is a slight color gradient visible, transitioning from redder hues in the central region to slightly bluer tints in the outskirts. No prominent spiral arms, bars, or other distinct morphological features are discernible within the galaxy’s structure. There is no evidence of a major ongoing merger or tidal disturbance, although a subtle asymmetry might suggest a minor interaction in its recent history. Based on its apparent morphology, this galaxy could be classified as an elliptical galaxy.
