The galaxy presents as a single, dominant object with a smooth morphology. The galaxy exhibits a slightly elongated, almost round shape, leaning towards a lenticular classification. The light distribution appears centrally concentrated with a gradual decline in intensity towards the outer regions of the galaxy, exhibiting a notable lack of distinct spiral arm structures or prominent dust lanes. It has a generally homogenous color profile, with a faint yellow hue throughout. There is no apparent evidence of ongoing major merging activity or significant tidal disturbances, although some minor irregularities may be present upon further analysis. The galaxy appears relatively quiescent in terms of star formation, based on its color. The overall impression is of a mature and relatively undisturbed system.
