The galaxy presents as a moderately luminous, elongated object with a distinct central bulge. The morphology suggests an intermediate classification between elliptical and spiral, possibly an S0 type. The light distribution appears relatively smooth, with a concentration of older stars towards the core, indicated by the yellowish-orange hue. There's a hint of a flattened disk structure extending outwards, though defined spiral arms are not apparent. The disk exhibits a bluer color, suggesting the presence of a younger stellar population and ongoing star formation, albeit at a moderate rate. The galaxy shows some signs of minor tidal disturbances or interaction, possibly due to a nearby companion galaxy exhibiting a more spherical shape and similar yellow-orange hue. A slight asymmetry in the outer regions and a subtle warp in the disk further support this assessment. No prominent dust lanes are visible within the disk.
