The galaxy presents as a somewhat smooth, elliptical-shaped structure. It displays a concentrated, luminous core, indicative of a substantial central mass. The color profile is dominated by warmer tones, ranging from yellow to orange, suggesting a population of older stars with lower rates of active star formation. There's a subtle elongation to the galaxy's morphology, leaning towards a cigar-shaped appearance. No prominent dust lanes or spiral arm structures are visible, supporting the smooth classification. Very slight irregularities might be present, potentially indicating a past or ongoing minor interaction, but this is difficult to ascertain definitively from the image. The overall light distribution appears relatively uniform, with a gradual decrease in brightness moving from the core outwards.
