This galaxy presents an elliptical morphology when viewed from our vantage point. It exhibits a smooth luminosity gradient, with a bright, concentrated core region. The light profile suggests a centrally dominant population of older stars, contributing to the yellowish-white color observed near the core. The outer regions of the galaxy display a fainter, bluer hue, potentially indicating the presence of a younger stellar population or ongoing star formation within the galactic disk. There is evidence of disk-like structure. The orientation of the disk is highly inclined relative to our line of sight. No distinct spiral arms are visible, suggesting either a very tightly wound spiral structure or a more lenticular morphology. The overall shape is elongated, indicating significant flattening. There appear to be no major disturbances or signs of recent merger events, with smooth, regular outer isophotes.
