The galaxy presents a generally smooth appearance, with a concentrated central bulge. The ellipticity of the galaxy is noticeable; it appears somewhat elongated, with a cigar-like shape. The color profile indicates a higher concentration of older stellar populations, particularly in the central regions, with a yellowish hue. There is little evidence of distinct spiral arm structures or significant dust lanes. Marginal irregularities suggest the possibility of minor gravitational disturbances, although a major merging event is not readily apparent. Overall, the galaxy exhibits characteristics consistent with an elliptical or lenticular type.
