The galaxy presents as an elongated, elliptical structure with a smooth, diffuse light distribution, indicative of a significant spheroidal component. The core appears brighter and more condensed compared to the outer regions. Color gradients are subtle but noticeable, with the central bulge exhibiting a slightly yellower hue, potentially suggesting an older stellar population and higher metallicity. The bluer color in the outer regions is indicative of ongoing or recent star formation. There is a slight asymmetry to the overall shape, which could be due to a weak tidal interaction or internal dynamics. There are indications of what appears to be minor disturbances. The galaxy exhibits a red shift value that places it at a considerable distance. Estimated size is about 6 kpc.