The observed galaxy exhibits an elliptical morphology with a high degree of central concentration. The primary color appears to be reddish-yellow, becoming more diffuse and redder towards the outer regions. The galaxy lacks any distinct spiral arm structure or noticeable dust lanes, suggesting a relatively smooth distribution of stars. The galaxy appears nearly circular in projection, indicating a minimal inclination angle relative to the line of sight. There is no strong evidence of ongoing major merger activity, although subtle irregularities in the outer regions could point to minor gravitational interactions or tidal disturbances. The overall appearance is consistent with that of an early-type galaxy, possibly an elliptical galaxy that has largely exhausted its supply of gas and dust, resulting in a reduced rate of star formation.
