The galaxy appears as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. The core exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. Fainter, diffuse light extends outwards from the core, gradually fading into the background. No distinct spiral arm structures or prominent dust lanes are visible. There are hints of blue light in the outer regions. The overall appearance suggests a galaxy that is potentially spheroidal or elliptical in nature, with no signs of ongoing major mergers or significant disturbances. 
