The galaxy presents as a concentrated, somewhat elongated spheroid. The light distribution is dominated by a smooth, centrally concentrated bulge with a noticeable lack of distinct features such as spiral arms or prominent dust lanes. There might be a very subtle, diffuse disk component, but the spheroid dominates the overall structure. The color profile is generally uniform, with a suggestion of redder hues throughout the galaxy, indicative of an older stellar population. There is no obvious presence of ongoing major star formation; the stellar population is likely dominated by older, lower-mass stars. No signs of any tidal tails or other morphological disturbances are present, pointing to a dynamically relaxed and relatively isolated system. The galaxy does not appear to be undergoing any major mergers.
