The galaxy presents as a relatively smooth, elliptical or lenticular structure, exhibiting minimal discernible features such as spiral arms or a prominent disk. Its overall shape appears largely spheroidal with high central concentration. There is very little evidence of dust lanes. The galaxy's color gradient suggests a dominant population of older stars, with a more reddish hue concentrated towards the core region, transitioning to slightly bluer tones in the outer parts. The light distribution is relatively uniform, showing no indication of active star formation regions or prominent irregularities, it looks like it has been mostly quenched. There are signs of possible tidal disturbances and/or previous minor mergers, possibly explaining the irregular morphology. It would be beneficial to obtain spectra and conduct photometric analysis to determine a more detailed description of the star forming activity.
