The galaxy exhibits a generally smooth morphology, with a discernible, though not sharply defined, disk structure. The light distribution suggests a central bulge that appears yellowish-white, transitioning to a bluer hue in the outer regions of the disk. The apparent shape is elongated or cigar-shaped, indicating an elliptical or potentially an edge-on spiral structure. The galaxy appears relatively isolated with no obvious major merger events or tidal disturbances, but there may be minor asymmetry or disturbances present. The overall color profile suggests that the central regions are dominated by an older stellar population while the disk contains some younger, star-forming regions. The galaxy is of moderate size, with a diameter of approximately 4.5 kpc.
