The galaxy presents as a predominantly elliptical or spheroidal structure, exhibiting a high degree of smoothness in its overall appearance. It appears to be fairly compact, with an estimated effective radius of approximately 6.8 kpc. There is little evidence of significant disk-like features or spiral arms.

The color profile suggests a relatively old stellar population, with a redder overall hue. The galaxy is not showing any clear indications of ongoing major mergers or significant tidal disturbances, though a very faint disturbed feature can be inferred. The galaxy appears to be in a relatively quiescent state concerning star formation.
