The galaxy appears as a centrally concentrated, elliptical-like object. Its color profile suggests a dominant population of older stars, inferred from the yellowish hue, with a possible red shift. The galaxy exhibits a relatively smooth, featureless morphology. No distinct spiral arms, bars, or prominent dust lanes are discernible at this resolution, indicating a lack of significant ongoing star formation in the outer regions. There is no clear evidence of major tidal disturbances or ongoing mergers, although some minor asymmetry cannot be ruled out. The overall shape is between a circle and a cigar shape.
