The galaxy presents as a moderately bright, disk-shaped system with an approximate visual diameter of ~5 kpc. The overall color profile suggests a mature stellar population, with a relatively bright, yellowish central bulge dominating the light output. The disk exhibits a bluer hue, possibly indicating ongoing star formation. The disk itself appears relatively smooth, with no distinct spiral arm structure readily apparent in the image. The morphology is intermediate, leaning towards a less defined disk structure. There is no significant evidence of tidal disturbances, major mergers, or strong gravitational interactions visible in the image. The galaxy appears generally undisturbed.
