The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The color profile suggests an older stellar population, with a dominant yellowish hue indicating a prevalence of evolved stars. There are no obvious spiral arm structures or prominent dust lanes visible. A slight asymmetry might suggest a minor gravitational interaction or recent accretion event. A faint, diffuse object to the left might be a tidal tail, perhaps from this interaction, or a smaller galaxy in the process of merging. Overall, the galaxy presents a well-defined, slightly elongated structure.
