The galaxy presents a predominantly smooth, round morphology. There is a concentration of light towards the center, suggestive of a bulge component. The color profile indicates a redder hue overall, potentially suggesting an older stellar population and a lower rate of ongoing star formation within the observed bands. There is a slight asymmetry to the light distribution. Although it presents as largely undisturbed, there is a subtle suggestion of a very minor tidal interaction occurring. The galaxy appears relatively compact given its estimated size.
