The galaxy presents as an elliptical morphology, though not perfectly spherical, exhibiting a slight elongation. The central region is characterized by a concentrated, bright yellowish-white glow, indicative of a dense stellar population, likely older stars. Moving outward from the core, the luminosity decreases gradually, and the color shifts to a slightly bluer hue, suggesting a younger stellar population in the outer regions or some low-level star formation. The galaxy's overall structure appears smooth, without any prominent spiral arms, bars, or irregular features. There is no obvious sign of any major mergers or tidal disruptions. The shape is primarily in between round and cigar shaped, appearing to be only slightly elliptical.
