The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated, displaying a bright, compact core that gradually fades into the surrounding halo. There is an absence of prominent spiral arms or distinct features like dust lanes. The color profile is relatively uniform, shifting toward the red end of the spectrum in contrast to what would be observed in younger galaxies. Overall, the galaxy has a spheroidal shape with a round structure. There is no sign of any major ongoing merging activity or tidal disturbances. The galaxy appears to be a fairly evolved, quiescent system, likely composed predominantly of older stellar populations. 
