The galaxy presents as a well-defined, oblate spheroid with a distinct disk-like structure observed edge-on. The central bulge exhibits a bright, concentrated luminosity gradient, suggestive of a dense stellar population. This central region transitions smoothly into a surrounding disk. The disk structure shows evidence of possible dust lanes, which can be seen as dark bands along its major axis. 

The overall color profile indicates a mixed stellar population, with the central bulge exhibiting a yellower, older stellar population, and the disk showing bluer hues. The overall morphology suggests a possible disturbed state and a recent or ongoing merger. The galaxy displays evidence of tidal features or faint streamers extending from the main body, further corroborating the potential interaction.
