The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a significantly higher luminosity, suggesting a concentrated nucleus or bulge. A gradual decrease in luminosity is observed moving outwards from the core, with no distinct spiral arm features visible. The color profile appears slightly red-shifted, indicating a population of older stars and a relatively low rate of ongoing star formation within the galaxy. No significant tidal distortions or merging features are apparent, suggesting a gravitationally stable system. The galaxy appears well-rounded, with a minor axis ratio close to unity.
