The galaxy presents as a relatively compact object, exhibiting a smooth, symmetrical morphology. It appears roughly elliptical in shape, with a high degree of roundness, lacking any obvious spiral arm structures or pronounced disk features. The galaxy's light profile is centrally concentrated, suggesting a dominant bulge component. There is a lack of evidence for significant tidal disturbances, ongoing mergers, or prominent star-forming regions. The colour index, derived from observations in g, r, and z bands, suggests a moderate red colour, potentially indicative of an older stellar population.
