The galaxy presents as an elongated, disk-like structure, suggesting a spiral or lenticular morphology viewed at a considerable angle. The central region exhibits a bright, concentrated luminosity, indicative of a prominent galactic bulge likely populated by older stellar populations. The colour of the bulge appears yellowish-orange, potentially indicating a greater abundance of older, redder stars. Extending outwards from the bulge are faint, diffuse structures that could be indicative of spiral arms. These arms are not well-defined but appear to exhibit a bluer hue, possibly due to the presence of younger, hotter stars and ongoing star formation regions. The galaxy displays some level of disturbance, evidenced by the irregular shape of the outer regions and subtle asymmetries in the overall structure. The overall appearance suggests the possibility of a minor merger event or tidal interactions with another galaxy. The rate of star formation within this galaxy appears to be relatively low, possibly due to the depletion of gas reserves.
