The galaxy presents as an elliptical or lenticular morphology, displaying a smooth light distribution without prominent spiral arms or a distinct bulge. The galaxy is elongated, appearing cigar-shaped with a high aspect ratio. The color profile shows a concentration of redder hues in the central region, possibly indicating an older stellar population, while the outer regions display bluer colors, suggesting the presence of younger, hotter stars. No significant tidal features or obvious signs of recent major merger events are apparent, although there may be minor asymmetry hinting at past interactions or internal disturbances. The overall structure suggests a relatively evolved galaxy that may be undergoing passive evolution with a moderate rate of star formation.
