The galaxy presents as an elongated, spindle-shaped object, suggesting an edge-on or nearly edge-on orientation. The central bulge appears relatively prominent with a yellowish hue, indicative of an older stellar population. The disk exhibits a bluer tint, potentially signifying ongoing star formation activity. There are no immediately obvious spiral arms. There is little visual evidence of any major mergers or significant tidal disturbances that would suggest any interaction with another galaxy. The overall impression is that of a fairly undisturbed, late-type disk galaxy.
