The galaxy presents as a somewhat elongated, disc-like structure. There's a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. Fainter spiral arms extend from the central region, displaying a bluer color indicative of ongoing star formation. The dust lanes are faint, but discernible within the disc, contributing to the irregular appearance of the arms. Overall, the galaxy exhibits a transitional morphology, somewhere between a pure elliptical and a well-defined spiral galaxy, hinting at a possible ongoing process of morphological transformation. There seems to be very minimal signs of tidal disturbances suggesting little interaction with other galaxies or any recent major merger event.
