The observed galaxy exhibits a generally smooth morphology, suggestive of an elliptical or lenticular classification. The galaxy appears elongated, with a discernible cigar shape. There is little evidence of strong spiral arm structures or distinct star-forming regions. A lack of major disturbances would indicate the galaxy has not experienced a recent major merger. The overall color profile indicates a population of older stars, and a low rate of star formation. The core is visibly brighter and more condensed than the outer regions.