The galaxy presents as a centrally concentrated object with an elliptical morphology. The core exhibits a bright, relatively uniform yellowish hue, suggesting an older stellar population. Extending outwards from the core, the luminosity gradually decreases. There is evidence of a faint, diffuse disk or extended halo surrounding the central bulge. The overall structure appears mostly undisturbed, with no strong signs of tidal interactions or recent mergers. Faint irregular patches surrounding the core are present, and may signify younger star forming regions. The galaxy displays a modest redshift, indicating a significant cosmological distance.
