The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a higher concentration of light, suggestive of a bulge or a bright nucleus. The color profile appears relatively smooth, with a gradient from a yellowish-white core to bluer hues towards the outer edges. The smoothness of the color and light distribution indicates a lack of prominent spiral arm structures or significant dust lanes. There appears to be minor disturbances, with the galaxy showing a slight asymmetry. Overall, the galaxy appears to be a relatively massive system, potentially with a low rate of star formation, exhibiting characteristics of a disk galaxy.
