The galaxy presents as a somewhat elongated, disk-like structure. Its color profile suggests a central bulge that is yellowish-white in appearance, indicating a population of older stars. The outer regions of the disk exhibit a bluer hue, suggestive of more recent or ongoing star formation. There is a very slight indication of spiral arm structure, but this is not strongly defined. The galaxy appears relatively undisturbed, without any major signs of ongoing mergers or tidal interactions. The overall light distribution is concentrated towards the center, gradually fading towards the edges of the disk. The shape suggests it is not a face-on spiral, but rather tilted at a significant angle relative to our line of sight, with an approximate estimated diameter of 5.75 kpc. Overall this is a relatively massive galaxy with limited current star formation. 
