The galaxy presents as an elliptical morphology, elongated with a high aspect ratio. Its major axis is significantly larger than its minor axis. The light distribution appears relatively smooth, lacking strong evidence of spiral arms or distinct features within the disk, suggesting a high Sersic index. There is a color gradient visible, shifting from a yellowish hue at the center to a redder hue towards the outer regions. This color gradient likely indicates a population of older, redder stars dominating the outer regions and a younger, bluer population at the center. There's no indication of ongoing major mergers or significant tidal disturbances, with the object appearing relatively undisturbed. The galaxy's angular size is small, implying it is a relatively small object or at a great distance.
