The galaxy presents an elliptical morphology, appearing elongated in shape. The central bulge exhibits a concentrated luminosity with a yellowish hue, suggesting an older stellar population. Moving outward from the core, the galaxy's light gradually fades into a more diffuse halo. There appears to be a slight distortion or irregularity at the lower edge of the galaxy, potentially indicating a minor interaction or disturbance. Overall, the galaxy seems to be relatively smooth in structure, with no prominent spiral arms visible. It is oriented with its major axis at an angle, revealing an overall flattened appearance.
