The galaxy presents an elliptical morphology, appearing relatively smooth and centrally concentrated. A pronounced central bulge is observed, exhibiting a yellowish hue, indicative of an older stellar population. Moving outward from the core, the galaxy's luminosity gradually decreases, with a subtle transition toward a redder color in the outer regions. There is very little evidence of distinct spiral arm structure or significant dust lanes. The overall form appears largely undisturbed, lacking prominent tidal features or morphological peculiarities that might suggest recent major mergers. The galaxy's shape is moderately flattened, displaying an intermediate axis ratio. There are no discernible signs of active star formation regions or pronounced blue knots within the galaxy's structure. The galaxy appears to be relatively isolated, with no obvious companion galaxies in close proximity within the observed field.
