The galaxy presents a generally smooth, elliptical morphology. Its shape is elongated, approximating a cigar-like form when projected on the sky. The light profile suggests a centrally concentrated spheroid, with no apparent spiral arm structures or distinct disk features.

The galaxy exhibits a color gradient, trending towards a yellow hue, with the central region appearing more luminous than the outer edges. This may suggest an older stellar population dominating the overall light. There is a slight color variation at the outer edges that suggest some possible ongoing low levels of star formation, however.

Based on its red shift, the galaxy is relatively distant. There is no evidence of any significant ongoing mergers or tidal disturbances from the image.
