The galaxy presents as a centrally concentrated elliptical, exhibiting a smooth, diffused morphology. It possesses a generally rounded shape, with only minor deviations from perfect circularity. The light distribution suggests a well-defined core region, possibly indicating the presence of a supermassive black hole at the center. 

There's a colour gradient within the galaxy; the central region shows a distinct reddish hue, suggestive of an older stellar population. The outer regions appear to be slightly bluer in comparison, hinting at the existence of younger, hotter stars.

There is no visible spiral arm structure or significant dust lane obscuration, suggesting the galaxy has undergone significant processing of gas and dust and/or is past the peak star formation. No evidence of a major ongoing merger is observed; however, there's some minor irregularity in the outer regions, potentially signifying a recent or ongoing minor interaction.
