The galaxy presents a somewhat elliptical morphology. The central bulge appears smooth and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the light fades gradually into a less defined, fainter halo, indicating a diffuse distribution of stars. The disk structure, if present, appears to be viewed close to edge-on. No distinct spiral arms or prominent dust lanes are discernible. The overall impression is that of a relatively quiescent galaxy, likely a late-type spiral or an elliptical galaxy, viewed at a distance where fine details are blurred. The lack of blue light and defined structure suggests moderate levels of on-going star formation.
