The galaxy presents as a moderately bright, relatively compact object with a generally elliptical morphology. The light distribution appears smooth, lacking distinct spiral arm structures or prominent star-forming regions. The central region exhibits a yellowish-orange hue, suggesting an older stellar population likely dominated by evolved stars. Moving outward from the core, the color transitions subtly to a slightly bluer halo, possibly indicating the presence of a younger stellar population at lower densities. The overall smooth appearance suggests a lack of ongoing major mergers or significant tidal disturbances, although subtle asymmetries cannot be ruled out at this resolution. It appears to be an early-type galaxy. 
