The galaxy presents as an elongated, spindle-shaped object. It exhibits a relatively smooth morphology, with no discernible spiral arms or bar structure visible. The color profile suggests a more evolved stellar population, with a generally reddish-yellow hue indicating older stars and potentially dust obscuration. There appears to be a slight concentration of light towards the center, suggesting the presence of a central bulge or nucleus. The overall structure indicates a possible elliptical or lenticular galaxy type, with a lack of significant ongoing star formation apparent in the color and smoothness. There is a very slight asymmetry to the galaxy's shape, with the right side appearing slightly thicker than the left. There is no evidence of a major merger event.
