The object presents as a somewhat compact galaxy with a generally smooth morphology. The light distribution appears centrally concentrated, exhibiting a soft gradient in surface brightness outwards. No distinct spiral arm structures or a well-defined disk component are discernible; however, subtle irregularities may indicate minor structural disturbances. Color gradients suggest a population gradient, with the central regions appearing yellower and the outer regions showing hints of bluer light. The overall color profile indicates the presence of both older stellar populations and possibly some ongoing star formation, contributing to the galaxy's luminosity across multiple wavelengths. The galaxy appears relatively isolated, although higher resolution images would be needed to confirm the absence of faint tidal features or nearby companion galaxies.
