The galaxy appears to be an elliptical type, presenting with a smooth, concentrated light profile. The central region exhibits a bright, yellowish hue, suggesting an older stellar population and relatively low levels of current star formation. The overall shape is elongated, approaching a cigar-like form rather than a perfect sphere. There is no discernable spiral structure or significant dust lane visible in the image. Faint extensions of light are observed, suggesting a moderate halo or envelope extending beyond the main body of the galaxy. The galaxy does not exhibit obvious signs of recent or ongoing merger activity, such as tidal tails or strong distortions in its morphology. The estimated size of the galaxy is approximately 4.6 kpc. The galaxy is observed at a redshift of approximately 0.218. Based on its redshift and color indices, it is considered a moderately luminous galaxy, with an estimated mass of approximately 10^10.7 solar masses.
