The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical or lenticular type. The central region exhibits a high concentration of light, appearing bright and yellowish-white. The galaxy displays a generally round shape, with only a slight deviation towards an elongated form. There is limited evidence of spiral arm structures or significant dust lanes. Faint bluish-white regions can be observed, hinting at areas of possible recent star formation, although they are not highly prominent. The galaxy does not appear to be undergoing any major merging activity, although some minor disturbances or interactions with smaller companions cannot be ruled out due to the presence of slight irregularities in the outer regions. The overall color profile suggests an older stellar population with lower levels of on-going star formation relative to its mass.
