The galaxy presents as an elliptical or lenticular type, exhibiting a predominantly smooth morphology with a slight degree of elongation. The central region displays a concentrated luminosity gradient, suggesting a significant stellar population density. The color profile transitions from a yellowish core to a subtly redder outer halo. There is little evidence of distinct spiral arms or significant dust lanes. A slight asymmetry is observed in the light distribution, which may indicate minor tidal interactions or internal disturbances. Overall, the galaxy appears to be a relatively evolved system, with a low rate of star formation and a substantial stellar mass.
