The galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a bright, somewhat diffuse glow, suggesting a high density of stars in the central region. Moving outward from the core, the luminosity gradually decreases, with no distinct spiral arms or disk structures readily apparent in the image. The overall shape appears nearly circular, with minimal deviation from a perfect ellipse. The color profile indicates a dominance of redder wavelengths across the galaxy, implying an older stellar population with relatively low ongoing star formation. There is very little evidence of dust lanes or active star-forming regions within the visible structure. The outer regions fade smoothly into the background sky, indicating a gradual decline in stellar density and a lack of sharp edges or tidal features.
