The galaxy presents as a well-defined, elliptical structure, elongated along its major axis. The central bulge exhibits a smooth, concentrated brightness, with a yellowish hue suggesting a population of older stars. The disk appears relatively thin and inclined, with the spiral arms not distinctly resolved. The overall color profile shifts from a more yellow-red in the center to a slightly bluer tone in the outer regions.

A faint, irregular feature extends from one end of the galaxy, potentially indicative of a tidal tail or disrupted satellite galaxy. This extension displays a bluer color, hinting at the presence of younger, hotter stars, possibly resulting from recent star formation. No significant dust lanes are clearly visible within the disk. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger or interaction.
