The galaxy presents as a single, smooth object with a concentrated central region. Its overall shape appears close to round. There is a slight gradient in color, with the core exhibiting a yellowish-orange hue, suggesting an older stellar population or significant dust obscuration. Moving outward from the core, the colors transition to a redder and fainter halo, possibly indicative of a less dense stellar distribution. There is no evidence of spiral arms, bars, or any significant disturbances or tidal features. The galaxy appears isolated, with no signs of ongoing or recent merger activity. Overall, based on its morphology and color profile, this galaxy could be classified as an elliptical galaxy.
