The galaxy presents as an elongated, cigar-shaped structure, potentially an elliptical or lenticular galaxy viewed at an oblique angle. The central region exhibits a yellowish hue, indicative of an older stellar population. The outer regions transition to a bluer color, suggesting the presence of younger, hotter stars and potentially some ongoing star formation. The galaxy appears relatively smooth in texture, with no immediately obvious signs of spiral arms or significant dust lanes. The overall appearance suggests a galaxy that is not currently undergoing a major merging event, but the slight asymmetry could indicate a past or minor interaction. The object subtends an angular size that is small, suggesting it is a distant object.
