This galaxy appears to be a relatively face-on spiral or lenticular galaxy with a smooth central bulge. The disk component is visible, exhibiting a slightly elongated shape. There is no evidence of distinct spiral arms, but a faint, mottled texture can be discerned, suggesting the presence of some substructure within the disk. The color profile indicates a concentration of older stellar populations in the central bulge, indicated by the redder hue, while the disk shows bluer tones, potentially signifying regions of ongoing or recent star formation. No obvious signs of a major merger event are apparent, though subtle disturbances or interactions cannot be ruled out based on this image alone. The galaxy appears to be relatively isolated.
