The galaxy presents as a well-defined elliptical shape, exhibiting a smooth, concentrated light profile characteristic of an early-type system. It appears somewhat elongated, showing a cigar-like structure. The color gradients suggest a redder core transitioning to slightly bluer outer regions. This color variation may indicate differing stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars contributing to the outer regions. No obvious spiral arm structures or dust lanes are discernible. The lack of prominent features and the smooth overall appearance support a classification favoring an elliptical galaxy experiencing a relatively low rate of star formation. There is no morphological evidence of significant ongoing or recent merger activity.
