The galaxy presents as a slightly elongated, centrally concentrated object. A prominent, diffuse central bulge exhibits a warm hue, suggesting an older stellar population and relatively low levels of current star formation within this region. Surrounding the bulge, a fainter, bluer disk or extended halo is visible. The blue color implies the presence of younger, hotter stars, and potentially some ongoing star formation. The overall morphology suggests a relatively smooth structure, with no obvious signs of strong spiral arms or major disturbances. The object may be an early-type spiral galaxy, viewed at an oblique angle, or potentially an elliptical galaxy with some residual star formation. There are hints of minor asymmetry or a faint tidal feature, possibly indicating a past or ongoing minor merger event. 
