The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a somewhat elliptical morphology, with the semi-minor axis approximately 70% of the semi-major axis. The color gradient is subtle, with the central region appearing slightly bluer than the outer regions. There is no evidence of prominent spiral arms or a distinct bar structure. The overall impression is that of a galaxy with a relatively uniform stellar population. The galaxy is likely a disk galaxy with some form of bulge, but the lack of detailed visible structure is somewhat unclear and may be due to seeing conditions or its angle relative to our perspective. No current signs of disturbances due to merging are present.
