This galaxy presents as an elongated, elliptical morphology. The light distribution shows a smooth, concentrated core with a gradual decrease in intensity outwards. The galaxy appears to be significantly inclined relative to our line of sight. The color profile suggests a relatively red population, potentially indicating an older stellar population with ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible in the image. The galaxy has a hint of being disturbed, however it appears there is no major merging involved. The overall structure indicates a moderate concentration.
