The galaxy presents a generally smooth morphology. Its overall shape appears elliptical, though not perfectly so, exhibiting a slight elongation. The light profile appears centrally concentrated, with a gradual decrease in intensity outward from the core. The color is predominantly yellow/orange, indicative of an older stellar population with fewer young, hot, blue stars, and a likely lack of significant ongoing star formation. There are suggestions of minor irregularities in the outer regions, possibly hinting at past or ongoing interactions. The internal structure appears relatively uniform without prominent dust lanes or spiral arm features visible at this resolution.
