The galaxy presents as a centrally concentrated, elongated structure. Its overall morphology appears relatively smooth, suggesting it is likely an elliptical galaxy with an old stellar population. There is little evidence of spiral arms or significant dust lanes. The color profile suggests a redder hue, consistent with older stars and a lower rate of star formation. No tidal features or signs of ongoing mergers are readily apparent. The galaxy exhibits a high degree of ellipticity, appearing cigar-shaped.