The galaxy appears as an elongated, ellipsoidal structure. The central region exhibits a concentrated luminosity, suggesting the presence of a prominent galactic nucleus. The color profile indicates a predominantly yellow-orange hue in the central bulge, potentially indicative of an older stellar population with lower rates of ongoing star formation. Fainter, diffuse green emissions are detected in the galaxy's outer regions. The outer regions have a relatively smooth texture. There are no visible spiral arms or other prominent features, which suggests this galaxy might be classified as an elliptical or lenticular galaxy. The aspect ratio suggests a significant inclination relative to the observer's line of sight. There is no visual evidence of any ongoing major mergers or tidal disturbances.
