The galaxy presents as a luminous, moderately compact object, approximately 6 kiloparsecs in radius. Its morphology is primarily smooth, with a dominant spheroidal component. There is evidence of a possible interaction or merger event, indicated by a slight asymmetry and potential tidal features or disturbances in its outer regions.

The core of the galaxy appears to be dominated by older stellar populations, suggesting a relatively low specific star formation rate. The color indices suggest it emits strongly across the visible spectrum, with a peak in the red, indicating that it may be an elliptical galaxy. There is evidence of ongoing star formation with a low presence of bluer colors in some regions. The estimated mass of the galaxy is substantial, placing it within the range of typical elliptical galaxies.
