The galaxy presents as a centrally concentrated object with a predominantly smooth morphology. The overall shape appears nearly round. There is a subtle color gradient noticeable, transitioning from a bluer hue at the core to slightly redder tones in the outer regions. Evidence of spiral arms or distinct features like bars is absent, suggesting a lack of significant, ongoing star formation in a defined disk. The galaxy appears relatively undisturbed, showing no clear signs of major merging activity or tidal disruption. The light distribution appears relatively uniform, without prominent knots or star-forming regions. The galaxy has an estimated size, with an effective radius of several kiloparsecs. The integrated light suggests that the galaxy is of intermediate luminosity.
