The galaxy presents a lenticular morphology, appearing as a smooth, elongated structure. The central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a high density of stars in this region. The color profile transitions from a yellowish-white core to a more diffuse, reddish-tinged outer region. The lack of defined spiral arms or distinct dust lanes suggests minimal ongoing star formation. There is no visual evidence of any major mergers or tidal disturbances in the galaxy's morphology. The galaxy's overall smooth appearance indicates that it may be in a more quiescent state of stellar evolution.
