The galaxy presents as a somewhat elliptical, diffuse structure, though not perfectly round. A bright, concentrated central region dominates the luminosity profile, suggesting a prominent galactic nucleus. The outer regions exhibit a fainter, more irregular morphology with some asymmetry, possibly hinting at minor tidal disturbances or recent interactions. The color distribution appears relatively uniform, with a yellowish hue indicating a population of older stars. There is little evidence of distinct spiral arms or significant dust lanes. Star formation appears subdued, with a lack of prominent blue regions typically associated with young, massive stars.
