The galaxy presents a smooth, elongated morphology, indicative of an elliptical or lenticular type. Its color profile suggests a moderate redshift. The central region exhibits a high surface brightness, appearing as a concentrated spheroid with a yellowish hue, possibly representing an older stellar population. Fainter, bluer extensions are visible beyond the core, suggesting regions of more recent star formation or a diffuse stellar halo. The galaxy is moderately inclined to our line of sight. There is an appearance of a slight disturbance, though it is difficult to definitively determine. Overall, the galaxy appears to be a moderately massive system with ongoing star formation, but at a relatively low rate.
