The galaxy presents as a relatively smooth, elongated structure. It is not perfectly elliptical, displaying a slight asymmetry along its major axis, appearing somewhat cigar-shaped. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. Surrounding the central region, there is a bluish halo, potentially indicating ongoing star formation within a disk-like component. The outer edges of the galaxy are less defined, gradually fading into the background sky. No prominent spiral arm structures or bar features are distinctly visible. There is a hint of minor disturbance or a possible interaction event on one side of the disk component. Overall, the galaxy appears to be undergoing some evolutionary processes, but is currently fairly settled.
