The galaxy presents as a relatively smooth and centrally concentrated structure. It has an elliptical morphology, appearing somewhat cigar-shaped. The light profile suggests a higher concentration of older stars in the center, which glows a yellow-white. Moving outwards from the central bulge, the galaxy's light transitions to a slightly bluer hue, indicating the presence of younger, hotter stars. This blue component may represent a disk that cannot be fully resolved at this resolution or a population of younger stars. There are no prominent features, such as spiral arms or tidal tails, suggesting it has not undergone a recent major merger. Subtle asymmetry is present, though not indicative of an ongoing major interaction.
