The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. The color profile suggests a population of older stars, exhibiting a yellowish-red hue. There is little evidence of spiral arm structures or significant dust lanes. The galaxy displays a generally symmetrical shape, with a slight elongation, appearing somewhere between round and cigar-shaped. No obvious signs of recent or ongoing major merging events are apparent, though some minor disturbance is not out of the question. The galaxy presents an undisturbed structure, with a high degree of smoothness.
