The galaxy presents a primarily smooth morphology, with a significant fraction of light concentrated in a central bulge. The overall shape appears approximately round, though not perfectly spherical, exhibiting a slight elongation. While generally smooth, faint and subtle features are visible, potentially indicating the presence of a disk component or minor disturbances within the galaxy's structure. There is no obvious sign of strong tidal features, such as long tails or strong distortions suggesting an ongoing major merger. Color gradients are noticeable, with a central region appearing yellower than the outer regions which tend towards blue. This suggests the possibility of an older stellar population dominating the bulge, while bluer stars indicate regions of ongoing or recent star formation in the outer regions. The galaxy does not appear to be a pure elliptical but instead appears to have disk features that would make it fall somewhere on the lenticular to spiral spectrum. 
