The galaxy presents a generally smooth, elliptical morphology. There is a bright, concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding the core, there is a more diffuse halo that fades gradually into the background sky. There is very little evidence of distinct spiral arms or prominent dust lanes, or any sign of disk features. No significant tidal disturbances or indications of recent major merger events are apparent. The galaxy exhibits a moderate degree of roundness, with no clear cigar-shaped or highly elongated form. There may be faint features or subtle irregularities. However, at this resolution and depth, it’s difficult to definitively categorize it beyond a relatively undisturbed, smooth morphology.
