This galaxy, at a redshift of approximately 0.035, presents as a somewhat elongated, lenticular structure with a bright central bulge. The light distribution suggests a relatively smooth profile, although there is a hint of disturbed morphology. The galaxy appears to be undergoing some form of gravitational interaction, possibly a merger or tidal disruption. There is a faint blueish hue, particularly towards the outer regions, that may indicate some ongoing star formation, albeit at a low rate. The overall color is relatively uniform, suggesting a population of older stars and a moderate amount of dust. It is estimated to be approximately 2 kpc in radius.
