The galaxy presents a generally smooth morphology with a moderately elongated shape. The color profile suggests an older stellar population, primarily displaying reddish-yellow hues, particularly concentrated towards the central bulge. There is a subtle color gradient moving outwards from the core, transitioning to slightly bluer tones in the outer regions. This could be indicative of some ongoing, albeit low, star formation within the galaxy's disk. The disk itself appears relatively featureless, with no apparent spiral arm structure or significant dust lane obscuration visible at this resolution. There is no evidence of any major tidal disturbances or ongoing mergers, although minor irregularities cannot be ruled out. The overall impression is that of a relatively evolved galaxy, consistent with an intermediate redshift.
