The galaxy appears as a single, relatively smooth luminous object. The morphology suggests an elliptical galaxy type, with a generally round shape, although it is not perfectly spherical. There is little indication of spiral arms or a well-defined disk structure. The light distribution is centrally concentrated with a gradual fall-off in intensity toward the edges. Based on the colors, the stellar population appears to be dominated by older, redder stars, with little evidence of ongoing star formation. There is no visual evidence of significant tidal disturbances or interactions with other galaxies.
