The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, featureless morphology. The light profile is centrally concentrated, with a gradual decrease in surface brightness towards the outer edges. The shape is elongated, displaying a cigar-like appearance rather than a circular form. The central region exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluish light is visible in the outer regions, indicating the presence of some younger, hotter stars, although these are not prominent. There is no apparent evidence of spiral arms, a disk structure, or significant dust lanes. The overall structure suggests a relaxed system with minimal ongoing merger activity. No significant tidal features or morphological disturbances are observed.
