The galaxy presents as a luminous, elliptical morphology. It appears to be relatively smooth in texture with a concentrated central bulge. The color profile suggests a population dominated by older stars, as indicated by the yellowish hue. There may be a very slight disk structure, but this is not distinctly defined. No evidence of active star formation regions are visible. The overall structure indicates a high probability of a well-established, non-merging system that does not exhibit significant disturbances. The morphology appears somewhere between round and cigar-shaped, but is mostly in between.