The galaxy presents a generally smooth and elongated morphology. It appears to be an edge-on or highly inclined spiral or lenticular galaxy. There's a bright central bulge that gradually fades into a less luminous disk. The disk shows subtle color variations, with a bluer hue at the outer edges suggesting the presence of younger stellar populations or ongoing star formation. The redder tones concentrated towards the central region may indicate older stellar populations. There is no apparent evidence of spiral arm structure or prominent dust lanes from this vantage point. The overall light distribution is relatively even and undisturbed, suggesting a lack of recent major merger events, though subtle asymmetries cannot be entirely ruled out.
