The galaxy presents as a moderately bright object, exhibiting an elongated, cigar-shaped morphology. The light distribution suggests a relatively smooth structure, with a dominant bulge component that appears elliptical in shape. The central region of the galaxy displays a yellowish hue, possibly indicative of an older stellar population. A fainter, bluish component is observed adjacent to the main body, perhaps indicating a region of more recent star formation. There is a suggestion of minor gravitational disturbance, but the galaxy does not present with a classic merger morphology. Overall, this galaxy appears to be a fairly massive system, likely undergoing a moderate level of star formation.
