This galaxy appears to be a relatively small, lenticular system, likely an S0 type. It exhibits a smooth, centrally concentrated bulge that fades gradually into an extended disk. There are no prominent spiral arms visible, though a subtle, blueish hue is noticeable across the disk which indicates ongoing, but faint, star formation. The shape of the galaxy is elongated, suggesting that it is viewed at an angle, but not completely edge-on. The dust content is fairly low, judging by the lack of obscuration and the overall blueish appearance. The presence of a small disturbance in the form of a faint tail or tidal feature may indicate a recent minor merger event. The galaxy appears isolated.
