The galaxy presents an overall smooth morphology with a central bulge that dominates the light profile. There is a faint, elongated disc structure oriented vertically. The central bulge exhibits a bright, concentrated luminosity, suggesting a high stellar density. The galaxy displays a color gradient, appearing bluer towards the outer regions of the disc and more reddish/yellowish in the central bulge. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances; however, a slight asymmetry in the outer disc could indicate a past minor interaction. The overall appearance suggests a galaxy transitioning between a spiral and a lenticular type, potentially a disk galaxy nearing quiescence.
