This galaxy appears to be a lenticular or possibly an elliptical galaxy, exhibiting a smooth, elongated morphology. The color profile suggests a population of older stars, with the core appearing to be brighter and slightly more blueish. The overall light distribution is centrally concentrated with a gradual decrease in intensity towards the outer edges. The lack of prominent spiral arms or dust lanes supports the classification as a relatively evolved system, with little ongoing star formation. There is no indication of major merger activity or significant tidal disturbances. The shape is distinctly cigar-shaped.
