The galaxy presents as a relatively smooth, elongated structure. It appears to be an elliptical galaxy, exhibiting a notable lack of distinct spiral arms or features indicative of active star formation regions. The central bulge appears prominent and has a concentrated brightness. Moving outward from the center, the intensity of the light gradually decreases, suggesting a diminishing stellar density. The overall color of the galaxy is on the redder end of the spectrum, this suggests an older stellar population. There appears to be a slight flattening or elongation along one axis, transitioning from round to cigar-shaped. There is no visual evidence of any major mergers or tidal disturbances affecting the galaxy's overall morphology. The overall structure is consistent with that of a galaxy in its later stage of life.