The galaxy presents as a largely featureless elliptical or lenticular structure, exhibiting a smooth, concentrated luminosity profile. The central region is characterized by a bright, yellowish-white core, indicating a significant population of older stars. The overall shape appears close to circular. There's a notable absence of distinct spiral arms or prominent dust lanes. The outer regions gradually fade into the background sky, suggesting a smooth density gradient. The light is dominated by older stellar populations with minimal evidence of ongoing star formation. There is no visually apparent interaction with nearby galaxies. The light distribution appears regular, indicating it has not undergone any recent major mergers.
