The galaxy presents as a largely smooth, elliptical-like object with an apparent angular size that suggests it is relatively small. The galaxy exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards its outer regions. The core exhibits a yellowish-white hue, suggesting a dominant population of older stars. The outer regions of the galaxy show a slightly redder tint, possibly indicating a population of dust or a slightly older stellar population. No distinct spiral arms or prominent dust lanes are discernible within the observed image. The overall morphology suggests it could be an elliptical galaxy, or potentially a spiral galaxy seen at an angle where the spiral structure is not clearly resolved. There are slight hints of possible tidal disturbances, but the image is too blurry to determine exactly.
