The galaxy presents a somewhat elliptical morphology, displaying a centrally concentrated bulge that appears relatively smooth and dominates the overall light profile. There is a hint of an extended disk structure, faintly visible and oriented at an angle relative to our line of sight. The disk shows very little, if any, evidence of spiral arm structure or prominent star-forming regions. The color of the bulge appears more yellow, suggestive of an older stellar population, while the disk appears slightly bluer, potentially indicating more recent, though subdued, star formation activity. There's no clear sign of significant tidal disturbances or ongoing merger events. The galaxy appears to be relatively isolated, residing within its own space, though it could have minor companions in its area.
