The galaxy presents a generally smooth morphology with a concentration of light towards the center, suggesting a significant bulge component. The overall color appears yellowish, indicative of a stellar population dominated by older, redder stars. There is no prominent disk structure visible, and the light distribution lacks clear spiral arm features. Subtle variations in color and brightness hint at some internal structure, possibly faint dust lanes or areas of differing stellar populations. Based on the overall form, this galaxy could be categorized as an elliptical or lenticular type. There is a possibility of a minor interaction or disturbance, as evidenced by the slight asymmetry in the outer regions.
