The galaxy presents as a relatively smooth, disk-shaped structure with an apparent redshift of approximately 0.087. The light distribution suggests a prominent bulge component, possibly indicating an older stellar population concentrated towards the center. The galaxy exhibits a slight elongation, hinting at a possible bar structure or tidal interaction, though no distinct features are visually apparent. The color index suggests a redder population overall, consistent with a galaxy undergoing less active star formation. The absence of bright, blue knots associated with ongoing star formation further supports this observation. No significant dust lanes are visible in this image. The galaxy is likely a relatively massive system, given its estimated luminosity. Based on its smooth morphology, it is unlikely to be undergoing a major merger event.
