The galaxy presents a predominantly smooth morphology, with a likely central bulge that appears nearly spherical. The light distribution suggests a moderately elliptical shape, but with a slight elongation.  A hint of disklike structure is discernible, though subtle. The colour profile indicates a stellar population with a redder hue concentrated in the central region, suggesting older stars, with bluer components, likely indicative of younger star formation, extending outwards from the centre.  There may be signs of minor disturbances or asymmetries in the outer regions, perhaps due to gravitational interactions, but there are no large scale mergers currently happening. Overall, the galaxy appears to be moderately massive with on-going star formation and a moderate specific star formation rate.
