The galaxy appears as a centrally concentrated, luminous object with a generally smooth morphology. The light distribution suggests a spheroidal shape. The color profile indicates a redder hue, particularly in the central regions, with a gradual shift to slightly bluer tones towards the outer edges of the visible light. No distinct spiral arms or prominent features are apparent, hinting at a morphology dominated by an older stellar population. The galaxy exhibits a compact structure, lacking evidence of significant tidal disturbances or ongoing major merger events.
