The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a concentrated, smoother appearance, suggesting a relatively old stellar population. There is a slight asymmetry to the structure with a possible arm like extension. The galaxy displays a color gradient, with the central region appearing redder and the outer regions showing hints of bluer hues, which could indicate some level of ongoing star formation in those areas, though it is likely subdued overall. There is no strong evidence of a major ongoing merger.
