The galaxy presents an overall elliptical morphology, appearing relatively compact in its observed dimensions. A bright, centrally concentrated region dominates the galaxy's appearance, suggesting a significant concentration of stars or a possible active galactic nucleus (AGN). This central region exhibits a notably smooth texture. The outer regions of the galaxy appear less luminous, with some subtle features that may indicate faint spiral arm segments or tidal disturbances, although the image resolution limits a definitive assessment. There is potential evidence of minor morphological disturbances or irregularities within the galaxy's structure, possibly indicating ongoing or recent interactions. The light distribution suggests a system that is broadly redder in the outer edges.
