This galaxy presents as a relatively smooth, centralized structure. The light profile suggests a spheroidal shape, with a high degree of central concentration. There is little evidence of significant spiral arm structure or a prominent disk. The galaxy's color appears somewhat intermediate between a bluer, star-forming galaxy and a redder, quiescent galaxy. This could indicate ongoing or recently ceased star formation, or a stellar population of intermediate age. A faint, extended halo or envelope may surround the brighter central region of the galaxy, suggesting the possible presence of a diffuse stellar component. Overall, the galaxy appears to be a moderately luminous and relatively isolated system, showing no strong signs of recent major interactions or mergers. Further analysis would be needed to determine the precise star formation rate and the morphology of the fainter outer regions.
