The galaxy presents as an elliptical morphology, with a smooth, centralized light distribution. There is a noticeable concentration of light towards the core, which emanates outward gradually. The color profile suggests a dominant older stellar population, with a yellow-reddish hue that indicates a reduced presence of young, hot, blue stars. No distinct spiral arms or other prominent features such as bars or rings are discernible, reinforcing the elliptical classification. There is no evidence of active star formation regions visible, with the overall appearance suggesting a relatively quiescent system. The object is somewhat round in shape. The overall impression is that of a galaxy undergoing little to no current interaction or merging activity.