The galaxy presents as a relatively compact and elongated structure, likely a disk galaxy viewed at an oblique angle. The central region exhibits a somewhat smoother texture, suggesting a bulge component with a higher concentration of older stars. There is a suggestion of spiral arm structure, however the resolution does not permit complete assessment. The galaxy displays color variation, with a slightly bluer tinge, indicating the presence of younger stellar populations. The estimated physical size is moderate. Overall, this appears to be a disk galaxy with a modest star formation rate.
