The galaxy presents as a relatively compact, unresolved object at a redshift of approximately 0.26. The light profile suggests a predominantly smooth morphology, indicating a lack of prominent spiral arms or distinct disk structures. The galaxy exhibits a roughly circular appearance, though slight deviations from perfect roundness may be present.

Color analysis reveals a spectrum that includes emission in the green, red, and blue parts of the spectrum. This spectral distribution suggests ongoing star formation activity within the galaxy. The absolute magnitudes infer it is a luminous galaxy. Overall mass estimates suggest that this is a massive galaxy. There is an absence of strong visual indicators of any major ongoing merger events or significant tidal disturbances.
