The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core displays a yellowish hue, indicative of an older stellar population dominating the light output. Moving outwards from the center, the color transitions subtly towards a reddish tinge, possibly suggesting a difference in stellar populations or dust content. The overall structure is elliptical in shape with no discernible spiral arm structure or prominent dust lanes visible at this resolution. The galaxy exhibits high central concentration with faint extensions. There is no indication of any ongoing major merger events or significant tidal disturbances affecting its shape. The observed characteristics point towards it being an early-type galaxy, most likely an elliptical or lenticular galaxy at a significant distance.
