The galaxy presents as a relatively compact and luminous object with a predominantly smooth morphology. There is a concentration of light towards the central region, indicating a possible bulge component. The overall shape approximates a circular form, with minimal deviation from radial symmetry. The colour profile suggests an older stellar population, with a dominant yellow hue. There is no discernible evidence of spiral arms, bars, or ongoing major merger activity. Faint blue tinges could indicate a small amount of recent star formation, but the rate is likely low. Overall the galaxy appears to be a fairly large, relatively quiescent system.
