The galaxy presents as a largely featureless, elliptical or spheroidal structure. It exhibits a high degree of central concentration of light, with a smooth luminosity gradient outwards from the core. The galaxy appears nearly circular in projection, indicating a low apparent ellipticity. There is little to no evidence of spiral arm structure or dust lanes. The color profile appears relatively uniform across the galaxy, showing a slightly redder hue, with a hint of yellow within the core. This suggests a stellar population dominated by older, evolved stars and a relatively low rate of ongoing star formation. There are no indications of any major mergers or tidal disturbances, and the overall morphology points towards a relatively quiescent and stable system.
