The galaxy presents as a relatively smooth, elliptical or lenticular structure with a centrally concentrated luminosity profile. It exhibits a soft, diffuse glow, suggesting an older stellar population. There is little evidence of spiral arms or distinct features, although minor asymmetry and possible irregularities can be seen, indicating some form of perturbation. The color is primarily a pale yellow-orange, consistent with a population of evolved stars and indicating a moderate redshift. There appears to be a slight deviation in roundness, potentially due to interactions or internal dynamics.
