The galaxy presents as a centrally concentrated, relatively smooth object with an elliptical morphology. The light distribution is dominated by a strong central bulge which appears to be largely spheroidal. There is a noticeable color gradient, with the central region exhibiting a more yellowish hue, suggesting an older stellar population compared to the slightly bluer, though still faint, outer regions. There may be a faint disk structure, but it's difficult to resolve with the data at hand. No prominent spiral arms or distinct dust lanes are readily visible. There is no visual indication of any ongoing major merger activity, though there is a slight distortion of the light profile, hinting at a possible past minor interaction or disturbance. The overall appearance suggests a galaxy with a significant stellar mass and a low star formation rate. The object is moderately distant, as indicated by its redshift.
