The galaxy presents as a relatively smooth object, lacking prominent spiral arm structures or a defined central bulge. Its overall shape is elongated and somewhat cigar-shaped. The light distribution appears diffuse, with a slight concentration towards the central region, suggesting a higher density of stars there. There is a subtle color gradient across the galaxy, trending from a bluer hue at the top to a somewhat redder hue at the bottom, though this is not strongly defined. There are no clear indications of significant ongoing star formation or recent merger activity. Overall, the galaxy appears to be an elliptical type.
