The galaxy presents as a relatively smooth, disk-shaped system. The central bulge region exhibits a concentrated, bright yellowish-white luminosity, indicative of an older stellar population. The disk surrounding the bulge appears moderately inclined to our line of sight, presenting a somewhat elliptical profile. There is a faint hint of spiral structure, but the arms are not well-defined. The overall color suggests a later-type spiral galaxy, though lacking prominent blue star-forming regions. The bulge appears to dominate the overall light output of the galaxy. There are no obvious signs of ongoing major merger activity, although some minor irregularities within the disk cannot be ruled out.
