The galaxy presents an elliptical morphology, characterized by a smooth and concentrated light distribution. The galaxy exhibits a slightly elongated form. The central region displays a brighter, more intensely illuminated core, gradually decreasing in luminosity towards the outer regions. Color gradients are subtle but visible, with the core exhibiting a yellowish-orange hue, possibly indicative of an older stellar population. The outer regions show a slight shift towards redder tones, further supporting the presence of evolved stars. There is no discernible spiral arm structure or evidence of significant dust lanes. Overall, the galaxy appears to be a relatively undisturbed system with minimal signs of ongoing star formation. There are no clear signs of a major merging event, but it is possible there is a minor disturbance causing the elongation.
