The galaxy presents as an elongated spheroid. Its color profile is dominated by a central region exhibiting a bluish-white hue, potentially indicating a population of relatively young, hot stars. The outer regions appear somewhat redder, which might represent an older stellar population, dust, or a combination thereof. The light distribution is smooth. No obvious spiral arm structures or dust lanes are discernible in this image. The galaxy does not show any visual signs of strong tidal disturbances or major ongoing mergers, though a very slight asymmetry hints towards a possible minor interaction or previous merger event. The galaxy appears to be fairly compact and moderately luminous.
