This galaxy presents as a flattened, somewhat elongated structure with a bright, concentrated central bulge. The galaxy exhibits a relatively smooth morphology, indicating a possible elliptical type, although a faint disk-like component is also suggested by the flattened shape. The color gradient shifts from a yellower central region to bluer outer edges. This could indicate an older stellar population concentrated in the core and younger, bluer stars in the outer regions. There is no definitive spiral arm structure visible in the image. The galaxy appears relatively undisturbed, showing no strong evidence of recent mergers or tidal interactions. The slight elongation suggests the possibility of a cigar-like shape. 
