The galaxy presents as a single, centrally concentrated object with a largely smooth morphology. There is no significant presence of spiral arms or a distinct disk structure visible, appearing primarily as an elliptical or spheroidal system. The color appears relatively uniform across the galaxy, with a slightly yellowish hue, potentially indicating a population of older stars with lower star formation rates. The lack of substantial blue coloration supports this assessment. There is little evidence of ongoing major merging events or tidal disturbances in its immediate vicinity. The overall form suggests a system dominated by a spheroid component, likely a giant elliptical galaxy.
